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The high energy X-ray probe (HEX-P): studying extreme accretion with ultraluminous X-ray sources

Introduction: Ultraluminous X-ray sources (ULXs) represent an extreme class of accreting compact objects: from the identification of some of the accretors as neutron stars to the detection of powerful winds travelling at 0.1–0.2 c, the increasing evidence points towards ULXs harbouring stellar-mass...

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Автори: Matteo Bachetti, Matthew J. Middleton, Ciro Pinto, Andrés Gúrpide, Dominic J. Walton, Murray Brightman, Bret Lehmer, Timothy P. Roberts, Georgios Vasilopoulos, Jason Alford, Roberta Amato, Elena Ambrosi, Lixin Dai, Hannah P. Earnshaw, Hamza El Byad, Javier A. García, Gian Luca Israel, Amruta Jaodand, Kristin Madsen, Chandreyee Maitra, Shifra Mandel, Kaya Mori, Fabio Pintore, Ken Ohsuga, Maura Pilia, Daniel Stern, George Younes, Anna Wolter
Формат: Artigo
Мова:Inglês
Опубліковано: Frontiers Media S.A. 2023-11-01
Серія:Frontiers in Astronomy and Space Sciences
Предмети:
ultraluminous X-ray sources
HEX-P
pulsars
black holes
accretion
spectra
Онлайн доступ:https://www.frontiersin.org/articles/10.3389/fspas.2023.1289432/full
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