Hot emission-line stars after 134 years of study. A personal view of current problems.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F01%3A01010082" target="_blank" >RIV/67985815:_____/01:01010082 - 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
Hot emission-line stars after 134 years of study. A personal view of current problems.
Original language description
A brief review of current problems in the research of hot emission-line stars is presented. Special attention is paid to problems of reliable determination of basic physical properties of underlying stars and to possible role of duplicity in the whole phenomenon.
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/ME%20402" target="_blank" >ME 402: Collaboration on a complex study of hot 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
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Interacting astronomers: A symposium on Mirek Plavec's favorite stars.
ISBN
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ISSN
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e-ISSN
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Number of pages
14
Pages from-to
9-22
Publisher name
Astronomical Institute
Place of publication
Ondrejov
Event location
Los Angeles [US]
Event date
Oct 21, 2000
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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