ZTF J0007+4804 is the first known hot subdwarf-white dwarf binary that exhibits SU UMa-type dwarf nova outbursts with a 108.72-minute orbital period.
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The authors produce a 3D tomographic reconstruction of Galactic cosmic-ray proton density from Fermi-LAT gamma-ray data and a gas model, finding a smooth distribution with moderate inner-Galaxy enhancement consistent with AMS-02 local measurements.
MWC 656 hosts a hot stripped star companion of 1.48 solar masses instead of a black hole.
Identifies 596 WD-MS binary candidates within 100 pc (497 new) by detecting NUV excess in Gaia sources and fitting SEDs to estimate WD temperatures and masses.
Dust depletion from UV spectra is associated with peaks in 3D extinction density maps to locate and chemically characterize local gas clouds at ~100 pc scales.
Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.
Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.
citing papers explorer
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Discovery of the first outbursting hot subdwarf binary: ZTF J0007+4804
ZTF J0007+4804 is the first known hot subdwarf-white dwarf binary that exhibits SU UMa-type dwarf nova outbursts with a 108.72-minute orbital period.
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A Three-Dimensional Tomographic Reconstruction of the Galactic Cosmic-Ray Proton Density
The authors produce a 3D tomographic reconstruction of Galactic cosmic-ray proton density from Fermi-LAT gamma-ray data and a gas model, finding a smooth distribution with moderate inner-Galaxy enhancement consistent with AMS-02 local measurements.
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Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
MWC 656 hosts a hot stripped star companion of 1.48 solar masses instead of a black hole.
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Revealing Unresolved White Dwarf-Main Sequence Binaries using Gaia DR3 and GALEX I. A Volume limited study of 100 pc
Identifies 596 WD-MS binary candidates within 100 pc (497 new) by detecting NUV excess in Gaia sources and fitting SEDs to estimate WD temperatures and masses.
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Connecting the dusty dots: dust depletion and extinction of local interstellar clouds
Dust depletion from UV spectra is associated with peaks in 3D extinction density maps to locate and chemically characterize local gas clouds at ~100 pc scales.
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Long-term optical variability of high-mass X-ray binaries. III. Polarimetry
Long-term polarimetric monitoring shows circumstellar disks in Be/X-ray binaries are smaller and denser than in isolated Be stars, with distortions often preceding giant X-ray outbursts.
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Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
654 WD-FGK binaries cataloged with mostly low-mass hot white dwarfs formed via binary interactions.
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Chemical signatures of planetary systems in their host stars. Near-infrared spectroscopy of four planet-hosting wide binaries
Planet-hosting wide binaries display diverse differential abundance trends with condensation temperature that are not universal across systems.