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

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...

Ausführliche Beschreibung

Bibliographische Detailangaben
Hauptverfasser: 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
Format: Artikel
Sprache:English
Veröffentlicht: IOP Publishing 2024-01-01
Schriftenreihe:The Astrophysical Journal
Schlagworte:
Neutron stars
Compact objects
Ultraluminous x-ray sources
Online Zugang:https://doi.org/10.3847/1538-4357/ad8b9c

Online

https://doi.org/10.3847/1538-4357/ad8b9c

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