Photometric observations and analysis of the close binary system DV Aquarii

Details Photometric observations and analysis of the close binary system DV Aquarii Photometric observations and analysis of the close binary system DV Aquarii

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pasp...97...62o&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 97, Jan. 1985, p. 62-66. Research supported by the Japa

Astronomy and Astrophysics

Astronomy

3

A Stars, Binary Stars, Light Curve, Subgiant Stars, Variable Stars, Electrophotometry, Stellar Spectrophotometry

Scientific paper

Photoelectric BV light curves of the close binary system DV Aqr are
presented. These light curves are analyzed with a synthesis method to
determine the photometric elements. Physical properties of the system
are briefly discussed. It is found that DV Aqr is a detached system
consisting of a late-A and a K-subgiant star.

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