Detecting the Black Hole Candidate Population in M51’s Young Massive Star Clusters: Constraints on Accreting Intermediate-mass Black Holes

Intermediate-mass black holes (10 ^2  <  M _BH  < 10 ^5 M _⊙ ) are an open question in our understanding of black hole evolution and growth. They have long been linked to dense star cluster environments, thanks to cluster dynamics, but there are a limited number of secure detections. We leverage exi...

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Автори:	Kristen C. Dage, Evangelia Tremou, Bolivia Cuevas Otahola, Eric W. Koch, Kwangmin Oh, Richard M. Plotkin, Vivian L. Tang, Muhammad Ridha Aldhalemi, Zainab Bustani, Mariam Ismail Fawaz, Hans J. Harff, Amna Khalyleh, Timothy McBride, Jesse Mason, Anthony Preston, Cortney Rinehart, Ethan Vinson, Gemma Anderson, Edward M. Cackett, Shih Ching Fu, Sebastian Kamann, Teresa Panurach, Renuka Pechetti, Payaswini Saikia, Susmita Sett, Ryan Urquhart, Christopher Usher
Формат:	Artigo
Мова:	Inglês
Опубліковано:	IOP Publishing 2025-01-01
Серія:	The Astrophysical Journal
Предмети:	Intermediate-mass black holes Compact objects Ultraluminous x-ray sources Young star clusters Star clusters
Онлайн доступ:	https://doi.org/10.3847/1538-4357/ad9d37
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