Spectral and light variability of Be Star 60 Cygni
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F00%3A00001393" target="_blank" >RIV/00216208:11320/00:00001393 - 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
Spectral and light variability of Be Star 60 Cygni
Original language description
Long-tem, medium and rapid spectral and light variations of the Be star 60 Cyg are documented and analysed. Possible binary nature is suggested and contraints of existing models are outlined.
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/GA205%2F94%2F0025" target="_blank" >GA205/94/0025: Fine Structure of Line Profiles (CQEB): Another Clue to the Be Phenomenon.</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2000
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
The Be Phenomenon in Early-Type Stars IAU Colloquium 175
ISBN
1-58381-045-5
ISSN
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e-ISSN
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Number of pages
4
Pages from-to
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Publisher name
Sheridan Books
Place of publication
Michigan
Event location
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Event date
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Type of event by nationality
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UT code for WoS article
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