Central Compact Objects in Supernova Remnants

Andrea De Luca (INAF/Iasf Milano; Iuss Pavia)

Central Compact Objects in Supernova Remnants

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arxiv 0712.2209 v1 pith:DOJVFT75 submitted 2007-12-13 astro-ph

Andrea De Luca (INAF/Iasf Milano , Iuss Pavia) This is my paper · ORCID

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keywords inssccoscentralcompactobjectsremnantssourcessupernova

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Central Compact Objects (CCOs) are a handful of soft X-ray sources located close to the centers of Supernova Remnants and supposed to be young, radio-quiet Isolated Neutron Stars (INSs). A clear understanding of their physics would be crucial in order to complete our view of the birth properties of INSs. We will review the phenomenologies of CCOs, underlining the most important, recent results, and we will discuss the possible relationships of such sources with other classes of INSs.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Evolution of Calvera and Descendants of Calvera-like Central Compact Objects
astro-ph.HE 2026-07 conditional novelty 4.0 of 10

Calvera and similar CCOs evolve in the fallback-disc model into long-lived ordinary radio pulsars that occupy an observed cluster above the pulsar death valley.

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