A magnetic white dwarf formed through a binary merger within 35 million years | Paper Citation Record

Observation b5d2d9d3-2bf0-4da3-8332-917cd71edb45 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

A magnetic white dwarf formed through a binary merger within 35 million years , " * write output.state after.block = add.period write newline

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.026372Z

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Observation a3d43085-2db9-4c50-bedd-8e6c3b16503b · outbound

This paper cites write newline.

A magnetic white dwarf formed through a binary merger within 35 million years write newline

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.042829Z

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Observation ee350484-7795-433b-9818-d0a4fc041c07 · outbound

This paper cites 9 H& 0 D2vH I `.

A magnetic white dwarf formed through a binary merger within 35 million years 9 H& 0 D2vH I `

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.059602Z

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Observation 4c88c4c1-de4d-4e8d-8a1a-8a79386dc9f6 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.105766Z

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Observation ebfe42be-8467-4979-b89a-d11677c0de23 · outbound

This paper cites 2020, title On the Spectral Evolution of Hot White Dwarf Stars.

A magnetic white dwarf formed through a binary merger within 35 million years 2020, title On the Spectral Evolution of Hot White Dwarf Stars

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.125076Z

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Observation 17ca0bde-4688-4144-a2eb-28da6a0dce5d · outbound

This paper cites 2017, title Measurements of Physical Parameters of White Dwarfs: A Test of the Mass-Radius Relation , The Astrophysical Journal, 848, 11, 10.3847/1538-4357/aa8bb6.

A magnetic white dwarf formed through a binary merger within 35 million years 2017, title Measurements of Physical Parameters of White Dwarfs: A Test of the Mass-Radius Relation , The Astrophysical Journal, 848, 11, 10.3847/1538-4357/aa8bb6

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.213602Z

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Observation d6563682-4d65-4c65-9b73-224f75a2905f · outbound

This paper cites C., Kulkarni , S.

A magnetic white dwarf formed through a binary merger within 35 million years C., Kulkarni , S

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.302358Z

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Observation 180fb8a7-fd1e-48d2-9ead-1e5eabf00ded · outbound

This paper cites K., & Ruiz , M.

A magnetic white dwarf formed through a binary merger within 35 million years K., & Ruiz , M

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.378725Z

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Observation a33f0880-1b08-48bf-9491-21ecd247ee77 · outbound

This paper cites G., Kerr , R., Curtis , J.

A magnetic white dwarf formed through a binary merger within 35 million years G., Kerr , R., Curtis , J

Reference 9

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.774107Z

Source-reported events for the cited work

correction dated 2023-06-29. Source: crossref record 10.3847/1538-3881/acda92->10.3847/1538-3881/ac93ff:correction, observed 2026-07-11T02:58:32.078842+00:00. This notice travels one citation hop only.

Observation 522c4726-3a5d-49fe-8dfb-fc59477f46fd · outbound

This paper cites P., Ferrario , L., Tout , C.

A magnetic white dwarf formed through a binary merger within 35 million years P., Ferrario , L., Tout , C

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.470720Z

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Observation 83498407-1feb-480c-a3b3-a81366a8c6ab · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 11

Resolution: verified exact; raw_fallback, observed 2026-08-05T13:06:36.135051Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 4a465112-3e33-4f61-a179-d3d39a2d66c2 · outbound

This paper cites B., Fuller , J., et al.

A magnetic white dwarf formed through a binary merger within 35 million years B., Fuller , J., et al

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.594073Z

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Observation 44cbe22e-5eda-4d21-a609-18e91c6b4040 · outbound

This paper cites A., Clayton , G.

A magnetic white dwarf formed through a binary merger within 35 million years A., Clayton , G

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.669359Z

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Observation d8e78919-be29-4213-84c7-809b6733da86 · outbound

This paper cites 2016, title Mesa Isochrones and Stellar Tracks (MIST).

A magnetic white dwarf formed through a binary merger within 35 million years 2016, title Mesa Isochrones and Stellar Tracks (MIST)

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.744917Z

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Observation 2692356e-102d-441a-944a-9c1533206769 · outbound

This paper cites A., Caiazzo, I., Cunningham, T., et al.

A magnetic white dwarf formed through a binary merger within 35 million years A., Caiazzo, I., Cunningham, T., et al

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.792210Z

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Observation be5f0c13-58c2-4a34-b34b-f3f11e365c6a · outbound

This paper cites D., Kalirai , J.

A magnetic white dwarf formed through a binary merger within 35 million years D., Kalirai , J

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.853915Z

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Observation 22fc3fe9-e522-42ca-be7c-ded8ccfab590 · outbound

This paper cites 2013, title Stellar Multiplicity , Annual Review of Astronomy and Astrophysics, 51, 269, 10.1146/annurev-astro-081710-102602.

A magnetic white dwarf formed through a binary merger within 35 million years 2013, title Stellar Multiplicity , Annual Review of Astronomy and Astrophysics, 51, 269, 10.1146/annurev-astro-081710-102602

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.894544Z

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Observation 51c13561-055e-4610-a53b-bbe199ce7283 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:31.986399Z

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Observation b0b11a5d-59cd-4e10-895f-c47c932cc0ff · outbound

This paper cites T., Bailey , J.

A magnetic white dwarf formed through a binary merger within 35 million years T., Bailey , J

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.058499Z

Source-reported events for the cited work

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Observation 7d85dd77-5c8e-4300-b262-3148a8ffc9c4 · outbound

This paper cites A., & Bildsten , L.

A magnetic white dwarf formed through a binary merger within 35 million years A., & Bildsten , L

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.151072Z

Source-reported events for the cited work

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Observation 8d58bf6e-7021-4aea-80c3-4ea53f9fe292 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.307069Z

Source-reported events for the cited work

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Observation bee2068f-b702-46ed-a68f-4206007a3a45 · outbound

This paper cites L., Sarro , L.

A magnetic white dwarf formed through a binary merger within 35 million years L., Sarro , L

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.380608Z

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Observation 0a3a7ce6-86a3-49e1-a2b8-103800f862bb · outbound

This paper cites 2012, title Double Degenerate Mergers as Progenitors of High-field Magnetic White Dwarfs , Astrophysical Journal, 749, 25, 10.1088/0004-637X/749/1/25.

A magnetic white dwarf formed through a binary merger within 35 million years 2012, title Double Degenerate Mergers as Progenitors of High-field Magnetic White Dwarfs , Astrophysical Journal, 749, 25, 10.1088/0004-637X/749/1/25

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.488475Z

Source-reported events for the cited work

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Observation 3dd31014-63c6-4b64-b422-abeda4b2260f · outbound

This paper cites A., Chen , X., et al.

A magnetic white dwarf formed through a binary merger within 35 million years A., Chen , X., et al

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.583334Z

Source-reported events for the cited work

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Observation 951570fd-ea7e-44fa-b161-6a0747aae8f6 · outbound

This paper cites A., Webbink , R.

A magnetic white dwarf formed through a binary merger within 35 million years A., Webbink , R

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.605263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 23f37b49-175f-4619-9066-b57253c3ab83 · outbound

This paper cites P., Tremblay , P.

A magnetic white dwarf formed through a binary merger within 35 million years P., Tremblay , P

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.714347Z

Source-reported events for the cited work

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Observation 073389e3-7a50-4b80-b729-0e0bb9272cef · outbound

This paper cites The first catalog of candidate white dwarf-main sequence binaries in open star clusters: A new window into common envelope evolution.

A magnetic white dwarf formed through a binary merger within 35 million years The first catalog of candidate white dwarf-main sequence binaries in open star clusters: A new window into common envelope evolution

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-08-05T13:06:35.681610Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 2efdc47c-6398-42b3-ad66-6c2c9ccd832c · outbound

This paper cites S., Schreiber , M.

A magnetic white dwarf formed through a binary merger within 35 million years S., Schreiber , M

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:32.908722Z

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Observation 0b129116-0b06-4466-82bf-a1e3f2e9d97c · outbound

This paper cites M., J rgensen , I., Allington-Smith , J.

A magnetic white dwarf formed through a binary merger within 35 million years M., J rgensen , I., Allington-Smith , J

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.021110Z

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Observation cd2fe1f8-6d65-4c30-ba97-8458afcc90b6 · outbound

This paper cites L., & Reffert , S.

A magnetic white dwarf formed through a binary merger within 35 million years L., & Reffert , S

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.108777Z

Source-reported events for the cited work

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Observation 4d06d185-b34c-402c-84ae-a49e24ac7f97 · outbound

This paper cites L., & Reffert , S.

A magnetic white dwarf formed through a binary merger within 35 million years L., & Reffert , S

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.195078Z

Source-reported events for the cited work

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Observation ff1327fa-1811-4d21-a32f-f7a54a43e2e7 · outbound

This paper cites R., Tout , C.

A magnetic white dwarf formed through a binary merger within 35 million years R., Tout , C

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.309994Z

Source-reported events for the cited work

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Observation b5ee5a4a-f63f-45af-aa51-a0c2eda3f3b0 · outbound

This paper cites 1990, title On the Consequences of Low-Mass White Dwarf Mergers , The Astrophysical Journal, 353, 215, 10.1086/168609.

A magnetic white dwarf formed through a binary merger within 35 million years 1990, title On the Consequences of Low-Mass White Dwarf Mergers , The Astrophysical Journal, 353, 215, 10.1086/168609

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.365955Z

Source-reported events for the cited work

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Observation a516c959-b48c-4eb0-b0b3-058f35590f02 · outbound

This paper cites 2024, title Massive White Dwarfs in the 100 pc Sample: Magnetism, Rotation, Pulsations, and the Merger Fraction , The Astrophysical Journal, 974, 12, 10.3847/1538-4357/ad6905.

A magnetic white dwarf formed through a binary merger within 35 million years 2024, title Massive White Dwarfs in the 100 pc Sample: Magnetism, Rotation, Pulsations, and the Merger Fraction , The Astrophysical Journal, 974, 12, 10.3847/1538-4357/ad6905

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.495923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7b76fca-21cf-46c9-ab94-0b12c98b093d · outbound

This paper cites 2025, title The 100 pc White Dwarf Sample in the SDSS Footprint.

A magnetic white dwarf formed through a binary merger within 35 million years 2025, title The 100 pc White Dwarf Sample in the SDSS Footprint

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.567856Z

Source-reported events for the cited work

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Observation 9805895a-29db-425d-8dce-0abf1bb9335d · outbound

This paper cites K., et al.

A magnetic white dwarf formed through a binary merger within 35 million years K., et al

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.620096Z

Source-reported events for the cited work

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Observation ace863c2-5d98-4319-bc94-5655b1871491 · outbound

This paper cites 2013, in Planets, Stars and Stellar Systems.

A magnetic white dwarf formed through a binary merger within 35 million years 2013, in Planets, Stars and Stellar Systems

Reference 37

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.624790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 19dc68a1-fdc3-4bec-be9b-0ac605aea5d4 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.732052Z

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Observation 0cb2b5e2-20a9-4206-92b2-b22bdc1cbf37 · outbound

This paper cites Y., Yagi , K., & Arras , P.

A magnetic white dwarf formed through a binary merger within 35 million years Y., Yagi , K., & Arras , P

Reference 39

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.610381Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 45e4de92-6134-43a4-b351-0f3e8c8fb8ea · outbound

This paper cites 2024, title Evolution and Final Fate of Solar Metallicity Stars in the Mass Range 7 15 M _.

A magnetic white dwarf formed through a binary merger within 35 million years 2024, title Evolution and Final Fate of Solar Metallicity Stars in the Mass Range 7 15 M _

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.879983Z

Source-reported events for the cited work

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Observation 323d1962-58d9-4165-9a6f-78009d6ab8c3 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:33.991605Z

Source-reported events for the cited work

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Observation a4fa7542-aa81-42d9-9123-56a503ce955f · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.084588Z

Source-reported events for the cited work

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Observation 22d14a8b-cc1a-401a-b529-c14798d5bc64 · outbound

This paper cites D., Curtis , J.

A magnetic white dwarf formed through a binary merger within 35 million years D., Curtis , J

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.168922Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9068a66f-4aad-419a-8a1e-99d0a209717d · outbound

This paper cites R., Dhillon , V.

A magnetic white dwarf formed through a binary merger within 35 million years R., Dhillon , V

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.280509Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea5ae04c-d126-48c9-ba24-f1205b119b69 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.341188Z

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Observation 80f2202a-d4e2-482a-9c2e-27265165628d · outbound

This paper cites 2021, title The TianQin project: Current progress on science and technology , Progress of Theoretical and Experimental Physics, 2021, 05A107, 10.1093/ptep/ptaa114.

A magnetic white dwarf formed through a binary merger within 35 million years 2021, title The TianQin project: Current progress on science and technology , Progress of Theoretical and Experimental Physics, 2021, 05A107, 10.1093/ptep/ptaa114

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.394746Z

Source-reported events for the cited work

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Observation bcf12a9f-33ef-4af6-9eda-b2d5f35cf88f · outbound

This paper cites T., Costa , G., Girardi , L., et al.

A magnetic white dwarf formed through a binary merger within 35 million years T., Costa , G., Girardi , L., et al

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.432803Z

Source-reported events for the cited work

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Observation da0e7c10-d1d7-4947-8c94-2ebdf14731b0 · outbound

This paper cites S., Metzger , B.

A magnetic white dwarf formed through a binary merger within 35 million years S., Metzger , B

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.471370Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 721cb9a5-e313-498d-8c38-db485f3125f9 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.506294Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9248e1fb-6650-4cf3-975e-057860353e5d · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 50

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.543938Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 8cc2fb57-bfff-4ed4-be84-f2d957516f3b · outbound

This paper cites B., Cohen , J.

A magnetic white dwarf formed through a binary merger within 35 million years B., Cohen , J

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.585282Z

Source-reported events for the cited work

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Observation 91a757af-db96-496e-b6bb-b552da2de3f9 · outbound

This paper cites 2011, title Modules for Experiments in Stellar Astrophysics (MESA) , , 192, 3, 10.1088/0067-0049/192/1/3.

A magnetic white dwarf formed through a binary merger within 35 million years 2011, title Modules for Experiments in Stellar Astrophysics (MESA) , , 192, 3, 10.1088/0067-0049/192/1/3

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.617957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f978002f-c047-4f25-b93b-230726d251d3 · outbound

This paper cites 2013, title Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars , , 208, 4, 10.1088/0067-0049/208/1/4.

A magnetic white dwarf formed through a binary merger within 35 million years 2013, title Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars , , 208, 4, 10.1088/0067-0049/208/1/4

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.663446Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2a54d145-a0d8-4756-a80d-d53d27016105 · outbound

This paper cites 2015, title Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions , , 220, 15, 10.1088/0067-0049/220/1/15.

A magnetic white dwarf formed through a binary merger within 35 million years 2015, title Modules for Experiments in Stellar Astrophysics (MESA): Binaries, Pulsations, and Explosions , , 220, 15, 10.1088/0067-0049/220/1/15

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.706095Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 437267f3-3072-4b34-9cd2-2347c5b493dd · outbound

This paper cites B., et al.

A magnetic white dwarf formed through a binary merger within 35 million years B., et al

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.731849Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0675f2c1-91fa-4995-99d3-e2b8119dd4e1 · outbound

This paper cites an unresolved cited work.

A magnetic white dwarf formed through a binary merger within 35 million years Unresolved cited work

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.777515Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 52d98687-f557-4b37-8688-006f42a0486b · outbound

This paper cites R., Buckley , D.

A magnetic white dwarf formed through a binary merger within 35 million years R., Buckley , D

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.823287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5a64623c-579c-4694-8c79-0c3d7f35fad2 · outbound

This paper cites 2023, title Uncovering new white dwarf open cluster associations using Gaia DR3 , Astronomy and Astrophysics, 678, A20, 10.1051/0004-6361/202245706.

A magnetic white dwarf formed through a binary merger within 35 million years 2023, title Uncovering new white dwarf open cluster associations using Gaia DR3 , Astronomy and Astrophysics, 678, A20, 10.1051/0004-6361/202245706

Reference 58

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.495836Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 4739d6de-269c-4480-ace9-dc6f22a2288d · outbound

This paper cites X., Hennawi , J., Cooke , R., et al.

A magnetic white dwarf formed through a binary merger within 35 million years X., Hennawi , J., Cooke , R., et al

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:34.908235Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1fa41afb-fc3a-4bb7-afd9-c30611322b4c · outbound

This paper cites 1977, title On the absolute scale of mass-loss in red giants.

A magnetic white dwarf formed through a binary merger within 35 million years 1977, title On the absolute scale of mass-loss in red giants

Reference 60

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T13:06:36.301648Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 98510364-7080-4e75-9de0-2dc45dc793c1 · outbound

This paper cites 2016, title Nine new open clusters within 500 pc from the Sun , Astronomy and Astrophysics, 595, A22, 10.1051/0004-6361/201629158.

A magnetic white dwarf formed through a binary merger within 35 million years 2016, title Nine new open clusters within 500 pc from the Sun , Astronomy and Astrophysics, 595, A22, 10.1051/0004-6361/201629158

Reference 61

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.480413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 895fe419-78f7-4650-ac95-45740701f4af · outbound

This paper cites 1994, Stationary Lines and White Dwarf Spectra (Berlin, Heidelberg: Springer Berlin Heidelberg), 89--108, 10.1007/978-3-642-78820-8_7.

A magnetic white dwarf formed through a binary merger within 35 million years 1994, Stationary Lines and White Dwarf Spectra (Berlin, Heidelberg: Springer Berlin Heidelberg), 89--108, 10.1007/978-3-642-78820-8_7

Reference 62

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.470770Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation e9aab0bc-e769-4131-b024-1b3aec9b302c · outbound

This paper cites 2021, title Evolutionary Models for the Remnant of the Merger of Two Carbon-Oxygen Core White Dwarfs , The Astrophysical Journal, 906, 53, 10.3847/1538-4357/abc87e.

A magnetic white dwarf formed through a binary merger within 35 million years 2021, title Evolutionary Models for the Remnant of the Merger of Two Carbon-Oxygen Core White Dwarfs , The Astrophysical Journal, 906, 53, 10.3847/1538-4357/abc87e

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:35.061399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 430783ab-0aff-4baf-a4cc-05c8b01e32fa · outbound

This paper cites P., Jao , W.-C., Henry , T.

A magnetic white dwarf formed through a binary merger within 35 million years P., Jao , W.-C., Henry , T

Reference 64

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.401647Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation e9153c8c-0c20-413e-bacc-3d68e649d13b · outbound

This paper cites A., Wickramasinghe , D.

A magnetic white dwarf formed through a binary merger within 35 million years A., Wickramasinghe , D

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:35.116081Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d42a2b39-a5fc-40a6-a009-0ee053aadeac · outbound

This paper cites A., Fontaine , G., et al.

A magnetic white dwarf formed through a binary merger within 35 million years A., Fontaine , G., et al

Reference 66

Resolution: verified exact; doi, observed 2026-08-05T13:06:35.328029Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 645ea960-2fa1-4099-ae0a-bec218000046 · outbound

This paper cites A., Jordan , S., et al.

A magnetic white dwarf formed through a binary merger within 35 million years A., Jordan , S., et al

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-05T13:06:35.191959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Coverage vector

Reference resolution

Outbound references

Pith citing papers