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Related papers: Where are the Intermediate Mass Black Holes?

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Intermediate mass black holes (IMBHs) are an (as yet) elusive class of black holes that are expected to lie in the $10^2-10^5\,M_{\odot}$ range, between the firmly established stellar-mass black holes and ${\gtrsim}10^6\,M_{\odot}$…

Astrophysics of Galaxies · Physics 2018-05-16 Filippos Koliopanos

This paper reviews the subject of intermediate-mass black holes (IMBHs) with masses between those of "stellar-mass" and "super-massive" black holes. The existence of IMBHs is a real possibility: they might plausibly have formed as remnants…

Astrophysics · Physics 2007-05-23 Roeland P. van der Marel

Intermediate-mass black holes (IMBHs), with masses between roughly $10^2\,M_\odot$ and $10^5\,M_\odot$, represent a largely uncharted component of the black-hole (BH) population. They are theoretically predicted to form in several…

Astrophysics of Galaxies · Physics 2025-12-17 R. Pascale , G. Battaglia

Intermediate-mass black holes (IMBHs), with masses in the range $100-10^{6}$ M$_{\odot}$, are the link between stellar-mass BHs and supermassive BHs (SMBHs). They are thought to be the seeds from which SMBHs grow, which would explain the…

Astrophysics of Galaxies · Physics 2017-05-30 Mar Mezcua

Black holes (BHs) with masses between 100 to 100,000 times the mass of the Sun ($\rm{M}_{\odot}$) are classified as intermediate-mass black holes (IMBHs), potentially representing a crucial link between stellar-mass and supermassive BHs.…

Astrophysics of Galaxies · Physics 2024-02-29 Abbas Askar , Vivienne F. Baldassare , Mar Mezcua

Intermediate-mass black holes (IMBHs) have masses of about 100 to 100,000 solar masses. They remain elusive. Observing IMBHs in present-day globular clusters (GCs) would validate a formation channel for seed black holes in the early…

Intermediate-mass black holes (IMBHs: masses between $100 - 10^{6} M_{\odot}$) historically comprise of an elusive population compared to stellar-mass and supermassive BHs. Recently IMBHs have started to be observed at the centers of…

Astrophysics of Galaxies · Physics 2019-06-19 Paramita Barai , Elisabete M. de Gouveia Dal Pino

The existence of black holes (BHs) with masses in the range between stellar remnants and supermassive BHs has only recently become unambiguously established. GW190521, a gravitational wave signal detected by the LIGO/Virgo Collaboration,…

Black holes are usually observed to be of stellar-mass or supermassive. By natural extension, there should be a population of Intermediate-Mass Black Holes (IMBHs: with mass between $100$ to $10^6 M_{\odot}$) in the Universe; which has…

Astrophysics of Galaxies · Physics 2020-06-24 Paramita Barai , Elisabete M. de Gouveia Dal Pino

Using the Next Generation Very Large Array (ngVLA), we will make a comprehensive inventory of intermediate-mass black holes (IMBHs) in hundreds of globular cluster systems out to a distance of 25 Mpc. IMBHs have masses of about 100 to…

Astrophysics of Galaxies · Physics 2018-06-18 J. M. Wrobel , J. C. A. Miller-Jones , K. E. Nyland , T. J. Maccarone

Intermediate Mass Black Holes (IMBHs) are a class of black holes with masses in the range $10^2 \div 10^5$ $M_\odot$, which can not directly derive from stellar evolution. Looking for these objects and estimating their abundance is…

Astrophysics of Galaxies · Physics 2023-12-12 A. Franco , A. A. Nucita , F. De Paolis , F. Strafella , M. Maiorano

Intermediate-mass black holes (IMBHs) of mass $M_{\bullet} \approx 10^{2} - 10^{5}$ solar masses, $M_{\odot}$, are the long-sought missing link between stellar black holes, born of supernovae, and massive black holes, tied to galaxy…

Astrophysics of Galaxies · Physics 2017-09-21 Tal Alexander , Ben Bar-Or

Intermediate-mass black holes (IMBHs) occupy the $ 10^2 - 10^5\,M_\odot $ range, but their existence remains poorly constrained. Only a few candidates have been suggested in dwarf galaxies, globular clusters, and LIGO-Virgo-Kagra…

Astrophysics of Galaxies · Physics 2025-10-10 Cristiano Ugolini

Observational searches for Intermediate Mass Black Holes (IMBHs), defined to have masses between 30 and 300,000 solar masses, provide limits which allow up to ten percent of what is presently identified as halo dark matter to be in the form…

High Energy Physics - Theory · Physics 2009-04-22 Paul H. Frampton

Nearly every massive galaxy harbors a supermassive black hole (SMBH) in its nucleus. SMBH masses are millions to billions $M_{\odot}$, and they correlate with properties of spheroids of their host galaxies. While the SMBH growth channels,…

Intermediate-mass black holes (IMBHs), with masses of hundreds to thousands of solar masses, will be unique sources of gravitational waves for LISA. Here we discuss their context as well as specific characteristics of IMBH-IMBH and…

Astrophysics · Physics 2010-04-21 M. Coleman Miller

Intermediate-mass black holes (IMBHs) are those between 100 and 10$^5$ solar masses ($M_{\odot}$); their formation process is debated. One possible origin is the growth of less massive black holes (BHs) via mergers with stars and compact…

Astrophysics of Galaxies · Physics 2024-06-12 Michiko S. Fujii , Long Wang , Ataru Tanikawa , Yutaka Hirai , Takayuki R. Saitoh

Intermediate mass black holes (IMBHs) with a mass between $10^{2}$ and $10^{5}$ times that of the sun, which bridges the {mass gap between the} stellar-mass black holes and the supermassive black holes, are crucial in understanding the…

High Energy Astrophysical Phenomena · Physics 2017-05-05 Yun-Feng Liang , Yuan-Zhu Wang , Hao Wang , Xiang Li , Yi-Ming Hu , Zhi-Ping Jin , Yi-Zhong Fan , En-Wei Liang , Da-Ming Wei

Intermediate mass black holes (IMBHs), with masses between 100 to 10^5 M_\odot, represent the link between stellar mass black holes and the supermassive black holes that reside in galaxy centers. While IMBHs are crucial to our understanding…

Astrophysics of Galaxies · Physics 2018-07-25 Jenna M. Cann , Shobita Satyapal , Nicholas P. Abel , Claudio Ricci , Nathan J. Secrest , Laura Blecha , Mario Gliozzi

Stellar-mass and supermassive black holes abound in the Universe, whereas intermediate-mass black holes (IMBHs) of ~10^2-10^5 solar masses in between are largely missing observationally, with few cases found only. Here we report the…

High Energy Astrophysical Phenomena · Physics 2025-01-17 C. -C. Jin , D. -Y. Li , N. Jiang , L. -X. Dai , H. -Q. Cheng , J. -Z. Zhu , C. -W. Yang , A. Rau , P. Baldini , T. -G. Wang , H. -Y. Zhou , W. Yuan , C. Zhang , X. -W. Shu , R. -F. Shen , Y. -L. Wang , S. -X. Wen , Q. -Y. Wu , Y. -B. Wang , L. L. Thomsen , Z. -J. Zhang , W. -J. Zhang , A. Coleiro , R. Eyles-Ferris , X. Fang , L. C. Ho , J. -W. Hu , J. -J. Jin , W. -X. Li , B. -F. Liu , F. -K. Liu , M. -J. Liu , Z. Liu , Y. -J. Lu , A. Merloni , E. -L. Qiao , R. Saxton , R. Soria , S. Wang , Y. -Q. Xue , H. -N. Yang , B. Zhang , W. -D. Zhang , Z. -M. Cai , F. -S. Chen , H. -L. Chen , T. -X. Chen , W. Chen , Y. -H. Chen , Y. -F. Chen , Y. Chen , B. Cordier , C. -Z. Cui , W. -W. Cui , Y. -F. Dai , H. -C. Ding , D. -W. Fan , Z. Fan , H. Feng , J. A. Garcia , J. Guan , D. -W. Han , D. -J. Hou , H. -B. Hu , M. -H. Huang , J. Huo , S. -M. Jia , Z. -Q. Jia , B. -W. Jiang , G. Jin , X. Kong , E. Kuulkers , W. -H. Lei , C. -K. Li , J. -F. Li , L. -H. Li , M. -S. Li , W. Li , Z. -D. Li , T. -Y. Lian , Z. -X. Ling , C. -Z. Liu , H. -Y Liu , H. -Q. Liu , J. -F. Liu , Y. Liu , F. -J. Lu , L. -D. Luo , J. Ma , X. Mao , H. -Y. Mu , K. Nandra , P. O'Brien , H. -W. Pan , X. Pan , G. -J. Qin , N. Rea , J. Sanders , L. -M. Song , H. Sun , S. -L. Sun , X. -J. Sun , Y. -Y. Tan , Q. -J. Tang , Y. -H. Tao , B. -C. Wang , J. Wang , J. -F. Wang , L. Wang , W. -X. Wang , Y. -S. Wang , Z. -X. Wang , Q. -W. Wu , X. -F. Wu , H. -T. Xu , J. -J. Xu , X. -P. Xu , Y. -F. Xu , Z. Xu , C. -B. Xue , S. -J. Xue , Y. -L. Xue , A. -L. Yan , X. -T. Yang , Y. -J. Yang , J. Zhang , M. Zhang , S. -N. Zhang , Y. -H. Zhang , Z. Zhang , Z. Zhang , Z. -L. Zhang , D. -H. Zhao , H. -S. Zhao , X. -F. Zhao , Z. -J. Zhao , J. Zheng , Q. -F. Zhu , Y. -X. Zhu , Z. -C. Zhu , H. Zou
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