CATCH ME IF YOU CAN: IS THERE A "RUNAWAY-MASS" BLACK HOLE IN THE ORION NEBULA CLUSTER?
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F12%3A10129560" target="_blank" >RIV/00216208:11320/12:10129560 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1088/0004-637X/757/1/37" target="_blank" >http://dx.doi.org/10.1088/0004-637X/757/1/37</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1088/0004-637X/757/1/37" target="_blank" >10.1088/0004-637X/757/1/37</a>
Alternative languages
Result language
angličtina
Original language name
CATCH ME IF YOU CAN: IS THERE A "RUNAWAY-MASS" BLACK HOLE IN THE ORION NEBULA CLUSTER?
Original language description
We investigate the dynamical evolution of the Orion Nebula Cluster (ONC) by means of direct N-body integrations. A large fraction of residual gas was probably expelled when the ONC formed, so we assume that the ONC was much more compact when it formed compared with its current size, in agreement with the embedded cluster radius-mass relation from Marks & Kroupa. Hence, we assume that few-body relaxation played an important role during the initial phase of evolution of the ONC. In particular, three-bodyinteractions among OB stars likely led to their ejection from the cluster and, at the same time, to the formation of a massive object via "runaway" physical stellar collisions. The resulting depletion of the high-mass end of the stellar mass function inthe cluster is one of the important points where our models fit the observational data. We speculate that the runaway-mass star may have collapsed directly into a massive black hole (M center dot greater than or similar to 100 M-circle do
Czech name
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Czech description
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Classification
Type
J<sub>x</sub> - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
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Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2012
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astrophysical Journal
ISSN
0004-637X
e-ISSN
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Volume of the periodical
757
Issue of the periodical within the volume
1
Country of publishing house
US - UNITED STATES
Number of pages
10
Pages from-to
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UT code for WoS article
000309052800037
EID of the result in the Scopus database
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