Observability of HOFNARs at SRG/eROSITA
Neutron stars can appear as sources of different nature. In this paper we address the observability of a hypothetical class of neutron stars—HOt and Fast Non-Accreting Rotators, HOFNARs. These objects are heated due to the r-mode instability. With surface temperatures ∼10<sup>6</sup> K they are expe...
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| Autors principals: | , , , , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
MDPI AG
2022-06-01
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| Col·lecció: | Universe |
| Matèries: | |
| Accés en línia: | https://www.mdpi.com/2218-1997/8/7/354 |
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