Disk Tracing for B[e] Supergiants in the Magellanic Clouds
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F15%3A00454698" target="_blank" >RIV/67985815:_____/15:00454698 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1051/eas/1571051" target="_blank" >http://dx.doi.org/10.1051/eas/1571051</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1051/eas/1571051" target="_blank" >10.1051/eas/1571051</a>
Alternative languages
Result language
angličtina
Original language name
Disk Tracing for B[e] Supergiants in the Magellanic Clouds
Original language description
B[e] supergiants are evolved massive stars with a complex circumstellar environment. A number of important emission features probe the structure and the kinematics of the circumstellar material. In our survey of Magellanic Cloud B[e] supergiants we focuson the [OI] and [CaII] emission lines, which we identified in four more objects.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GA14-21373S" target="_blank" >GA14-21373S: Unveiling the mass-loss history of evolved massive stars</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2015
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
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
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Number of pages
2
Pages from-to
229-230
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
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