Pregled bibliografske jedinice broj: 85337
Atmospheric thermal structure of a sample of M type giants
Atmospheric thermal structure of a sample of M type giants // Astrophysics and Space Science, 282 (2002), 743-747 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 85337 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Atmospheric thermal structure of a sample of M type giants
Autori
Jurdana-Šepić, Rajka ; Kotnik-Karuza, Dubravka
Izvornik
Astrophysics and Space Science (0004-640X) 282
(2002);
743-747
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
stars: M giants; stars: atmospheres; physical parameters: excitation temperature
Sažetak
Vibrational temperatures in the atmospheres of nine M type giants of luminosity class III and subtypes M2-M8 located in the Galactic plane have been determined from the $\gamma$ band system of the TiO molecule. The relationship between $T_{exc}$ and $T_{eff}$ has been established in agreement with the chosen $T_{eff}$ calibration scale. The deviation of $T_{exc}$ with recspect to $T_{eff}$ for our stars has been used as an indicator of the depth of the atmospheric layers in which the molecular bands are formed.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus