The F supergiants at high Galactic latitudes

Details The F supergiants at high Galactic latitudes The F supergiants at high Galactic latitudes

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..933k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, Oct. 1988, p. 933-939. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

8

F Stars, Stellar Atmospheres, Stellar Composition, Stellar Spectra, Supergiant Stars, Astronomical Catalogs, Asymptotic Giant Branch Stars, Open Clusters, Stellar Evolution

Scientific paper

The atmospheric parameters and chemical abundance pattern for F-supergiants distant from the galactic plane, and for F-supergiants, members of the open clusters, are determined by the model atmosphere method using high resolution spectra. The inclusion of F-supergiants from open clusters permitted to estimate the absolute magnitudes of F-supergiants at high galactic latitudes. The analysis confirms the suggestion that the high-latitude F-supergiants are the objects on the post asymptotic giant branch evolution stage.

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