Spectral and light variability of Be star 60 Cygni (CROSBI ID 475212)
Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
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
engleski
Spectral and light variability of Be star 60 Cygni
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.
nije evidentirano
nije evidentirano
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nije evidentirano
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nije evidentirano
Podaci o prilogu
280-283-x.
2000.
objavljeno
Podaci o matičnoj publikaciji
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)
Podaci o skupu
Nepoznat skup
poster
29.02.1904-29.02.2096
