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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3644
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dc.contributor.authorFerro, A. A-
dc.contributor.authorGiridhar, S-
dc.contributor.authorChavez, M-
dc.contributor.authorParrao, L-
dc.date.accessioned2008-09-16T14:10:25Z-
dc.date.available2008-09-16T14:10:25Z-
dc.date.issued1989-04-
dc.identifier.citationAstronomy and Astrophysics, Vol. 214, No. 1 - 2, pp. 123 - 130en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3644-
dc.description.abstractPhotometry 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.en
dc.language.isoenen
dc.publisherEuropean Southern Observatoryen
dc.relation.urihttp://ads.iucaa.ernet.in/abs/1989A%26A...214..123Aen
dc.subjectAstronomical Photometryen
dc.subjectF Starsen
dc.subjectStellar Compositionen
dc.subjectSupergiant Starsen
dc.subjectHalosen
dc.subjectOxygen Spectraen
dc.subjectStellar Luminosityen
dc.subjectStellar Magnitudeen
dc.subjectStellar Modelsen
dc.subjectUBV Spectraen
dc.titleA photometric study of F-type stars of high galactic latitudeen
dc.typeArticleen
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