Pregled bibliografske jedinice broj: 89095
Rapid Light Variations of the Bright Be Star φ Per
Rapid Light Variations of the Bright Be Star φ Per // 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. (ur.).
San Francisco (CA): The Astronomical Society of the Pacific, 2002. str. 254-255 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
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Naslov
Rapid Light Variations of the Bright Be Star φ Per
Autori
Sudar, Davor ; Ruždjak, Domagoj
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
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, 2002, 254-255
Skup
Radial and Nonradial Pulsations as Probes of Stellar Physics, IAU Colloquium 185
Mjesto i datum
Leuven, Belgija, 26.07.2001. - 31.07.2001
Vrsta sudjelovanja
Poster
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
.
Sažetak
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.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
