Analysis of the Light Variations of Bs-Aquarii

Details Analysis of the Light Variations of Bs-Aquarii Analysis of the Light Variations of Bs-Aquarii

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982basi...10..234k&link_type=abstract

Bulletin of the Astronomical Society of India V. 10, P. 234, 1982

Astronomy and Astrophysics

Astronomy

1

Scientific paper

An analysis of UBV light variations of BS Aqr is presented. Intrinsic (U-B) and (B-V) values are used to derive the temperature and surface gravity. The mean values are Teff = 7600 ± 100K and log geff = 3.8 ± 0.1. These values suggest that BS Aqr is a normal population I pulsating star and a member of δ Scuti group.

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