Do Neutron Star Ultraluminous X-Ray Sources Masquerade as Intermediate-mass Black Holes in Radio and X-Ray?

Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve as potential candidates for (sub-Eddington) intermediate-mass black holes. However, a total of eight ULXs have now been...

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Κύριοι συγγραφείς:	Teresa Panurach, Kristen C. Dage, Ryan Urquhart, Richard M. Plotkin, Jeremiah D. Paul, Arash Bahramian, McKinley C. Brumback, Timothy J. Galvin, Isabella Molina, James C. A. Miller-Jones, Payaswini Saikia
Μορφή:	Artigo
Γλώσσα:	Inglês
Έκδοση:	IOP Publishing 2024-01-01
Σειρά:	The Astrophysical Journal
Θέματα:	Neutron stars Compact objects Ultraluminous x-ray sources
Διαθέσιμο Online:	https://doi.org/10.3847/1538-4357/ad8b9c
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