Pregled bibliografske jedinice broj: 46751
Spectral and light variability of Be star 60 Cygni
Spectral and light variability of Be star 60 Cygni // The Be Phenomenon in Early-Type Stars, IAU Colloquium 175, ASP Conference Series, Vol 214 / Smith, M.A. ; Henrichs, H.F. ; Fabregat, J (ur.).
San Francisco (CA): Astronomical Society of the Pacific (ASP), 2000. str. 280-283 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
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Naslov
Spectral and light variability of Be star 60 Cygni
Autori
Koubsky, Pavel ; Harmanec, Petr ; Hubert, A.M ; Floquet, M ; Kubat, Jiri ; Ballereau, Dominique ; Božić, Hrvoje ; Chauville, J ; Holmgren, David ; Yang, Stephenson ; Cao, H ; Eenens, Philippe ; Huang, Lin ; Percy, John R
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
The Be Phenomenon in Early-Type Stars, IAU Colloquium 175, ASP Conference Series, Vol 214
/ Smith, M.A. ; Henrichs, H.F. ; Fabregat, J - San Francisco (CA) : Astronomical Society of the Pacific (ASP), 2000, 280-283
Skup
The Be Phenomenon in Early-Type Stars, IAU Colloquium 175
Mjesto i datum
Alicante, Španjolska, 28.06.1999. - 02.07.1999
Vrsta sudjelovanja
Poster
Vrsta recenzije
Međunarodna recenzija
Sažetak
The analysis of high S/N spectra and photometyric data of 60 Cyg shows that: (1) Pronounced long-term variations in spectra are accompanied with light variations. (2) The medium-term variations of RV could indicate that 60 Cyg is a spectroscopic binary. (3) Two independent structures dominate the rapid variability of both spectrum and light of the star.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
