B[e] stars: pre- versus post-main sequence evolution
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F10%3A00356539" target="_blank" >RIV/67985815:_____/10:00356539 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
B[e] stars: pre- versus post-main sequence evolution
Original language description
The classication of numerous Galactic B[e] stars is hampered by uncertain or unknown stellar parameters. In addition, Herbig B[e] stars and B[e] supergiants, both surrounded by dusty disks, show many spectroscopic similarities. We use the 12C/13C ratio,which drops drastically during stellar evolution, and show that the appearance of 13CO band emission is an unambiguous proof for a supergiant nature.
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/KJB300030701" target="_blank" >KJB300030701: B[e] supergiants: where is their place within the evolution of massive stars?</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2010
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Interferometric View on Hot Stars
ISBN
978-607-02-1317-5
ISSN
1405-2059
e-ISSN
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Number of pages
2
Pages from-to
69-70
Publisher name
Universidad Nacional Autonoma Mexico
Place of publication
Mexico City
Event location
Vi?a del Mar
Event date
Mar 2, 2009
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
000305162500025