Napredna pretraga

Pregled bibliografske jedinice broj: 85733

CH Cygni: A Symbiotic Star in Its Transition Phase to Quiescence


Kotnik-Karuza, Dubravka; Jurdana-Šepić, Rajka
CH Cygni: A Symbiotic Star in Its Transition Phase to Quiescence // Progress in European Astrophysics / Rodono, Marcello (ur.).
Catania: Italian astronomical society, 1995. str. 205-206 (poster, međunarodna recenzija, sažetak, znanstveni)


Naslov
CH Cygni: A Symbiotic Star in Its Transition Phase to Quiescence

Autori
Kotnik-Karuza, Dubravka ; Jurdana-Šepić, Rajka

Vrsta, podvrsta i kategorija rada
Sažeci sa skupova, sažetak, znanstveni

Izvornik
Progress in European Astrophysics / Rodono, Marcello - Catania : Italian astronomical society, 1995, 205-206

Skup
JENAM 95 (4th European and 39th Italian Astronomical Society Meeting)

Mjesto i datum
Catania, Italija, 1-7.09.1995.

Vrsta sudjelovanja
Poster

Vrsta recenzije
Međunarodna recenzija

Ključne riječi
Simbiotske zvijezde
(Symbiotic stars)

Sažetak
The transition period of symbiotic stars from the activity to the quiescent phase has not yet been sufficiently investigated. In order to establish the relation of such stars to the recurrent novae and, on the other side, to the normal stars of the same spectral type, it is important to follow the spectrum also during the quiescent phases. The behavior of the cool component of the symbiotic star CH Cygni over the two year period after its longest 1977-1986 outburst has been investigated in the optical spectral region. The results show that CH Cygni has been very close to the condition of optical quiescency and that the comparison with normal stars could predict its future behavior. The relevant physical parameters, such as excitation temperature and microturbulent velocity, of M type stars 30 Her and beta And have been taken for reference. The curve of growth method with refined fitting procedure has been used.

Izvorni jezik
Engleski



POVEZANOST RADA