A photometric study of F-type stars of high galactic latitude

Details A photometric study of F-type stars of high galactic latitude A photometric study of F-type stars of high galactic latitude

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...214..123a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 214, no. 1-2, April 1989, p. 123-130. Research supported by CONACYT, Ministry

Astronomy and Astrophysics

Astrophysics

13

Astronomical Photometry, F Stars, Stellar Composition, Supergiant Stars, Halos, Oxygen Spectra, Stellar Luminosity, Stellar Magnitude, Stellar Models, Ubv Spectra

Scientific paper

Photometry in the O I 7774 A line and the uvbybeta system is presented for a group of high Galactic latitude F-type luminosity type I stars. The results indicate that the candidates are high gravity near solar Fe/H abundance stars in or near the Galactic plane. It is suggested that the stars are not tracers of recent star formations in the halo, but are probable low mass stars of the old disk population which do not conform to the UU Herculis class. The star BD 45 deg 1872 is an exception and is probably a low mass star very similar to members of the UU Her group.

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