Self-shielding clumps in starburst clusters

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F17%3A00484232" target="_blank" >RIV/67985815:_____/17:00484232 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S174392131500900X" target="_blank" >http://dx.doi.org/10.1017/S174392131500900X</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S174392131500900X" target="_blank" >10.1017/S174392131500900X</a>

Result language
angličtina
Original language name
Self-shielding clumps in starburst clusters
Original language description
Young and massive star clusters above a critical mass form thermally unstable clumps reducing locally the temperature and pressure of the hot 107 K cluster wind. The matter reinserted by stars, and mass loaded in interactions with pristine gas and from evaporating circumstellar disks, accumulate on clumps that are ionized with photons produced by massive stars. We discuss if they may become self-shielded when they reach the central part of the cluster, or even before it, during their free fall to the cluster center. Here we explore the importance of heating efficiency of stellar winds.
Czech name
—
Czech description
—

Project
—
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2017
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Formation, evolution, and survival of massive star clusters
ISBN
9781107138179
ISSN
1743-9213
e-ISSN
—
Number of pages
2
Pages from-to
251-252
Publisher name
Cambridge University Press
Place of publication
Cambridge
Event location
Honolulu
Event date
Aug 11, 2015
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000456237800058

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