Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.136..351v&link_type=abstract
Astrophysics and Space Science (ISSN 0004-640X), vol. 136, no. 2, Aug. 1987, p. 351-361. CNR-supported research.
Astronomy and Astrophysics
Astrophysics
Stellar Evolution, Stellar Temperature, Atmospheric Models, Chemical Composition, Stellar Atmospheres
Scientific paper
A comparison of different curves of growth derived from available model atmospheres has been done. The authors found that, in the effective temperature range (4000 - 8500K), the differences between models with the same (Teff, log g) from different authors, do not affect the shape of the curve of growth. Moreover, the shifts needed to superpose the curves, for different elements, differ only slightly when models from different authors are used. Then, in the low-temperature and for the gravities the authors considered, the particular model atmosphere used to draw the curve of growth is not the main constrain of the method.
Rossi Luca
Villada M. M.
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