The variable star SA 106 1024

Details The variable star SA 106 1024 The variable star SA 106 1024

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990pasp..102.1382l&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 102, Dec. 1990, p. 1382-1386. Research supported by the

Astronomy and Astrophysics

Astronomy

7

Stellar Spectrophotometry, Variable Stars, Brightness Distribution, Stellar Color, Ubv Spectra

Scientific paper

SA 106 1024 was observed as a suspected variable star in a list of broad-band UBVRI photometric standard stars. It is shown to be a delta Scuti star with a period of 0.066686 day. The galactic coordinates are l=351.34 deg and b=52.38 deg (1950.0), placing the star well above the galactic plane. The absolute magnitude is Mv=+2.55, which together with the mean apparent magnitude of 11.58, leads to a distance of some 640 pc. This suggests that it is a member of the young disk population, although the difference between the objective-prism spectral type and the photometric spectral type indicates that it could also be a kind of halo star.

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