Wolf-Rayet stars - what we know and what we don't
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F24%3A00616839" target="_blank" >RIV/67985815:_____/24:00616839 - isvavai.cz</a>
Result on the web
<a href="https://hdl.handle.net/11104/0363818" target="_blank" >https://hdl.handle.net/11104/0363818</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.59849/2078-4163.2024.2.73" target="_blank" >10.59849/2078-4163.2024.2.73</a>
Alternative languages
Result language
angličtina
Original language name
Wolf-Rayet stars - what we know and what we don't
Original language description
Today, we have a sufficiently complete picture of what the Wolf-Rayet (WR) stars are. Predictions of stellar evolution theory are in a good agreement with their parameters, estimated from observational data using stellar atmospheres codes, predictions of population synthesis also agree well with number of known WR stars. This article provides an overview of the main historical milestones in the studies of WR stars, showing how we came to this understanding, and what questions are still unanswered.
Czech name
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Czech description
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Classification
Type
J<sub>ost</sub> - Miscellaneous article in a specialist periodical
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
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Name of the periodical
Astronomical Journal of Azerbaijan
ISSN
2078-4163
e-ISSN
2078-4171
Volume of the periodical
19
Issue of the periodical within the volume
2
Country of publishing house
AZ - AZERBAIJAN
Number of pages
18
Pages from-to
73-90
UT code for WoS article
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EID of the result in the Scopus database
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