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Intermediate Mass Black Holes : Their Motion and Associated Energetics
Joint Authors
Source
Advances in High Energy Physics
Issue
Vol. 2014, Issue 2014 (31 Dec. 2014), pp.1-8, 8 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2014-02-27
Country of Publication
Egypt
No. of Pages
8
Main Subjects
Abstract EN
There is a lot of current astrophysical evidence and interest in intermediate mass black holes (IMBH), ranging from a few hundred to several thousand solar masses.
The active galaxy M82 and the globular cluster G1 in M31, for example, are known to host such objects.
Here, we discuss several aspects of IMBH such as their expected luminosity, spectral nature of radiation, and associated jets.
We also discuss possible scenarios for their formation including the effects of dynamical friction, and gravitational radiation.
We also consider their formation in the early universe and also discuss the possibility of supermassive black holes forming from mergers of several IMBH and compare the relevant time scales involved with other scenarios.
American Psychological Association (APA)
Sivaram, C.& Arun, Kenath. 2014. Intermediate Mass Black Holes : Their Motion and Associated Energetics. Advances in High Energy Physics،Vol. 2014, no. 2014, pp.1-8.
https://search.emarefa.net/detail/BIM-508528
Modern Language Association (MLA)
Sivaram, C.& Arun, Kenath. Intermediate Mass Black Holes : Their Motion and Associated Energetics. Advances in High Energy Physics No. 2014 (2014), pp.1-8.
https://search.emarefa.net/detail/BIM-508528
American Medical Association (AMA)
Sivaram, C.& Arun, Kenath. Intermediate Mass Black Holes : Their Motion and Associated Energetics. Advances in High Energy Physics. 2014. Vol. 2014, no. 2014, pp.1-8.
https://search.emarefa.net/detail/BIM-508528
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-508528