Properties of Massive Stars in VVV Clusters

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00472947" target="_blank" >RIV/67985815:_____/15:00472947 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/eas/1571079" target="_blank" >http://dx.doi.org/10.1051/eas/1571079</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/eas/1571079" target="_blank" >10.1051/eas/1571079</a>

Result language
angličtina
Original language name
Properties of Massive Stars in VVV Clusters
Original language description
The evolution of massive stars is only partly understood. Observational constraints can be obtained from the study of massive stars located in young massive clusters. The ESO Public Survey VISTA Variables in the Via Lactea (VVV) discovered several new clusters hosting massive stars (Borrissova et al. 2011). We derive the stellar parameters of all targets as well as surface abundances for a subset of them. For the cluster with the largest number of objects, we establish firmly that the WN and WC stars were initially more massive than the O stars still present in the cluster.
Czech name
—
Czech description
—

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

Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Article name in the collection
Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
ISBN
9782759819072
ISSN
1633-4760
e-ISSN
—
Number of pages
2
Pages from-to
337-338
Publisher name
EDP Sciences
Place of publication
Les Ulis
Event location
Nice
Event date
Jun 8, 2015
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000370302700078

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