Pregled bibliografske jedinice broj: 99292
Properties of RR Tel Using SAC Method
Properties of RR Tel Using SAC Method // EDPS Conference Series in Astronomy and Astrophysics / Combes, F. ; Barret, D. ; Contini, T. ; Meynadier, F. ; Pagani, L. (ur.).
Lyon, Francuska: EDP Sciences, 2001. str. 203 - 204 (poster, međunarodna recenzija, cjeloviti rad (in extenso), znanstveni)
CROSBI ID: 99292 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Properties of RR Tel Using SAC Method
Autori
Friedjung, Michael ; Kotnik-Karuza, Dubravka ; Selvelli, Pierluigi
Vrsta, podvrsta i kategorija rada
Radovi u zbornicima skupova, cjeloviti rad (in extenso), znanstveni
Izvornik
EDPS Conference Series in Astronomy and Astrophysics
/ Combes, F. ; Barret, D. ; Contini, T. ; Meynadier, F. ; Pagani, L. - : EDP Sciences, 2001, 203 - 204
Skup
SF2A-2001: Semaine de l'Astrophysique Francaise
Mjesto i datum
Lyon, Francuska, 28.05.2001. - 01.06.2001
Vrsta sudjelovanja
Poster
Vrsta recenzije
Međunarodna recenzija
Ključne riječi
RR Tel; SAC method; fundamental parameters
Sažetak
The SAC method is a semi-empirical method for analysing the emission lines of ions which have a complicated spectrum like Fe^+. In this work it has been applied to the symbiotic binary RR Tel and we were able to obtain information on different population ratios, non-LTE effects, the radius of line formation and the column density. All results are consistent with line formation in the wind of the cool giant. A minimum mass loss rate was found for it.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
