[O/C] abundance ratio for cool giants from the receding tip of the stellar Galactic bar (CROSBI ID 484282)
Prilog sa skupa u zborniku | sažetak izlaganja sa skupa | međunarodna recenzija
Podaci o odgovornosti
Kotnik-Karuza, Dubravka ; Jurdana-Šepić, Rajka ; Pavlenko, Yakiv
engleski
[O/C] abundance ratio for cool giants from the receding tip of the stellar Galactic bar
We identified the TiO bands and measured their intensity jumps in the near infrared spectra of ten M giants located in the Galactic plane. The correlation between the measured intensity jumps and spectral subtypes for particular TiO bands has been compared to the correlation established by use of the corresponding values calculated from model atmospheres for different &#61531 ; O/C&#61533 ; abundance ratios.
TiO molecular spectra; M giants
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
nije evidentirano
Podaci o prilogu
180-x.
2000.
objavljeno
Podaci o matičnoj publikaciji
Abstract book IAU 24 (24th General Assembly of the International Astronomical Union)
Manchester: International Astronomical Union
Podaci o skupu
IAU 24 (24th General Assembly of the International Astronomical Union)
poster
20.08.2000-27.08.2000
Manchester, Ujedinjeno Kraljevstvo