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[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

Kotnik-Karuza, Dubravka ; Jurdana-Šepić, Rajka ; Pavlenko, Yakiv [O/C] abundance ratio for cool giants from the receding tip of the stellar Galactic bar // Abstract book IAU 24 (24th General Assembly of the International Astronomical Union). Manchester: International Astronomical Union, 2000. str. 180-x

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

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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

Povezanost rada

Fizika