Formation mechanisms of IMBH in globular clusters
Giersz, M. ; Leigh, N. ; Hypki, A. ; Askar, A. LU
and Lützgendorf, N.
(2016)
In Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society
87.
p.555-558
- Abstract
- We very briefly discuss proposed in the literature possible scenarios for intermediate mass black holes formation in globular clusters. We also discuss the results of the MOCCA simulations of about 2000 models (BigSurvey) regarding the distribution of events connected with electromagnetic and gravitational radiations, namely: mass transfer on IMBH, collisions and mergers with IMBH and mergers with IMBH due to gravitational radiation. The rates of these events are very small, so their observation is very improbable.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/ab99c2e7-7fe3-4878-a3df-f913f30fe434
- author
- Giersz, M.
; Leigh, N.
; Hypki, A.
; Askar, A.
LU
and Lützgendorf, N.
- publishing date
- 2016
- type
- Contribution to journal
- publication status
- published
- subject
- keywords
- Stars: black holes, star clusters: general, Methods: numerical
- in
- Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society
- volume
- 87
- pages
- 4 pages
- publisher
- Italian Astronomical Society
- external identifiers
-
- scopus:85019411977
- ISSN
- 1824-016X
- language
- English
- LU publication?
- no
- id
- ab99c2e7-7fe3-4878-a3df-f913f30fe434
- alternative location
- https://openaccess.leidenuniv.nl/bitstream/handle/1887/47702/555.pdf?sequence=1
- date added to LUP
- 2018-10-30 18:02:04
- date last changed
- 2022-06-21 14:28:53
@article{ab99c2e7-7fe3-4878-a3df-f913f30fe434,
abstract = {{We very briefly discuss proposed in the literature possible scenarios for intermediate mass black holes formation in globular clusters. We also discuss the results of the MOCCA simulations of about 2000 models (BigSurvey) regarding the distribution of events connected with electromagnetic and gravitational radiations, namely: mass transfer on IMBH, collisions and mergers with IMBH and mergers with IMBH due to gravitational radiation. The rates of these events are very small, so their observation is very improbable.}},
author = {{Giersz, M. and Leigh, N. and Hypki, A. and Askar, A. and Lützgendorf, N.}},
issn = {{1824-016X}},
keywords = {{Stars: black holes, star clusters: general, Methods: numerical}},
language = {{eng}},
pages = {{555--558}},
publisher = {{Italian Astronomical Society}},
series = {{Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society}},
title = {{Formation mechanisms of IMBH in globular clusters}},
url = {{https://openaccess.leidenuniv.nl/bitstream/handle/1887/47702/555.pdf?sequence=1}},
volume = {{87}},
year = {{2016}},
}