Rapid Light Variations of the Bright Be Star φ Per (CROSBI ID 484851)
Prilog sa skupa u zborniku | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Sudar, Davor ; Ruždjak, Domagoj
engleski
Rapid Light Variations of the Bright Be Star φ Per
φ Per (HD 10516, HR 496) is a well known spectroscopic Be binary, with a 126.7-day period, which consists of B0.5IV primary ana a compact secondary (Gies et al., 1998). Its complex photometric behaviour including the long-term, phase locked and rapid light variations are described in Bozic et al. (1995). For the rapid variations they disclosed a formal 0.66-day period while from HIPPARCOS Hp photometry Hubert & Floquet (1998) found the value of 0.470 days.
.
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
Podaci o prilogu
254-255-x.
2002.
objavljeno
Podaci o matičnoj publikaciji
Radial and Nonradial Pulsations as Probes of Stellar Physics, IAU Colloquium 185, ASP Conference Proceedings, Vol. 259.
Aerts, C. ; Bedding, T. R. ; Christensen-Dalsgaar, J.
San Francisco (CA): The Astronomical Society of the Pacific
Podaci o skupu
Nepoznat skup
poster
29.02.1904-29.02.2096
