Central Compact Objects in Supernova Remnants
Andrea De Luca (INAF/Iasf Milano, Iuss Pavia)
TL;DR
This paper reviews the phenomenology of Central Compact Objects in supernova remnants, highlighting recent findings and exploring their potential links to other isolated neutron star classes.
Contribution
It provides a comprehensive review of CCOs, emphasizing recent observational results and discussing their possible evolutionary relationships with other neutron star types.
Findings
Recent CCO observations reveal diverse X-ray properties.
CCOs may represent a distinct class of young neutron stars.
Potential evolutionary links between CCOs and other INSs are discussed.
Abstract
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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