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CHEMICAL COMPOSITION OF COOL GIANT STARS

Based upon the catalogue of equivalent widths of absorption lines in spectra of cool giant - stars created at the Astrospectroscopy Department of the Astronomical Observatory in Odessa the abundances in their atmospheres is determined. This determination was made by using the method of model atmosph...

Whakaahuatanga katoa

I tiakina i:
Ngā taipitopito rārangi puna kōrero
Ngā kaituhi matua: N. S. Komarov, N. J. Basak, T. I. Gorbaneva, L. E. Kantsen
Hōputu: Artigo
Reo:Inglês
I whakaputaina: Odessa I. I. Mechnykov National University 2017-07-01
Rangatū:Odessa Astronomical Publications
Urunga tuihono:http://oap.onu.edu.ua/article/view/105750
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