Pregled bibliografske jedinice broj: 208738
Temperatures in the atmosphere of the cool component of CH Cygni
Temperatures in the atmosphere of the cool component of CH Cygni // Spectroscopically and spatially resolving the components of close binary stars / Hilditch, Ronald.W. ; Hensberge, Herman ; Pavlovski, Krešimir (ur.).
San Francisco (CA): Astronomical Society of the Pacific (ASP), 2004. str. 371-373
CROSBI ID: 208738 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Temperatures in the atmosphere of the cool component of CH Cygni
Autori
Jurdana-Šepić, Rajka ; Kotnik-Karuza, Dubravka ; Majlinger, Zlatko ; Pavlenko, Yakiv V.
Vrsta, podvrsta i kategorija rada
Poglavlja u knjigama, znanstveni
Knjiga
Spectroscopically and spatially resolving the components of close binary stars
Urednik/ci
Hilditch, Ronald.W. ; Hensberge, Herman ; Pavlovski, Krešimir
Izdavač
Astronomical Society of the Pacific (ASP)
Grad
San Francisco (CA)
Godina
2004
Raspon stranica
371-373
ISBN
1-58381-179-6
Ključne riječi
CH Cyg, optical spectrum, late-type star, TiO absorption, temperature
Sažetak
We have investigated the temperatures in the atmosphere of the cool component of CH Cygni by use of highly resolved optical and near infrared spectra taken in a short epoch of the 1998-2000 active phase. TiO absorption bands belonging to α , γ , γ ', β , δ , φ and ε band systems with partly resolved rotational structure have been studied and vibrational temperatures belonging to γ 'and φ system were obtained from the relative intensities of vibrational band heads. In order to determine the effective temperature we used model atmospheres appropriate for M giants and computed synthetic spectra by line-to-line approach. Results have been discussed in view of the previously determined rotational temperature.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
