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

dc.contributor.author	Ferro, A. A
dc.contributor.author	Giridhar, S
dc.contributor.author	Chavez, M
dc.contributor.author	Parrao, L
dc.date.accessioned	2008-09-16T14:10:25Z
dc.date.available	2008-09-16T14:10:25Z
dc.date.issued	1989-04
dc.identifier.citation	Astronomy and Astrophysics, Vol. 214, No. 1 - 2, pp. 123 - 130	en
dc.identifier.issn	0004-6361
dc.identifier.uri	http://hdl.handle.net/2248/3644
dc.description.abstract	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.	en
dc.language.iso	en	en
dc.publisher	European Southern Observatory	en
dc.relation.uri	http://ads.iucaa.ernet.in/abs/1989A%26A...214..123A	en
dc.subject	Astronomical Photometry	en
dc.subject	F Stars	en
dc.subject	Stellar Composition	en
dc.subject	Supergiant Stars	en
dc.subject	Halos	en
dc.subject	Oxygen Spectra	en
dc.subject	Stellar Luminosity	en
dc.subject	Stellar Magnitude	en
dc.subject	Stellar Models	en
dc.subject	UBV Spectra	en
dc.title	A photometric study of F-type stars of high galactic latitude	en
dc.type	Article	en