Star Clusters Triggered by GS242-03+37
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00522696" target="_blank" >RIV/67985815:_____/19:00522696 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S1743921318008578" target="_blank" >http://dx.doi.org/10.1017/S1743921318008578</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921318008578" target="_blank" >10.1017/S1743921318008578</a>
Alternative languages
Result language
angličtina
Original language name
Star Clusters Triggered by GS242-03+37
Original language description
We explore the Milky Way supershell GS242-03+37. We argue that the observed HI distribution can be explained as an expanding structure about 100 Myr old powered with a modest energy released by an OB association. The formation of star clusters has been triggered less than 30 Myr ago when the ISM density in the supershell increased due to the galactic differential rotation. The observed age sequence of young star clusters is related to the evolution of the column density during the supershell expansion.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2019
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Origins: From the Protosun to the First Steps of Life
ISBN
9781108471602
ISSN
1743-9213
e-ISSN
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Number of pages
2
Pages from-to
279-280
Publisher name
Cambridge University Press
Place of publication
Cambridge
Event location
Vienna
Event date
Aug 20, 2018
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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