The eclipsing binary BW Draconis

Details The eclipsing binary BW Draconis The eclipsing binary BW Draconis

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..97..337r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 97, no. 2, Dec. 1983, p. 337-351.

Astronomy and Astrophysics

Astrophysics

3

Astronomical Catalogs, Eclipsing Binary Stars, Light Curve, Stellar Spectrophotometry, Spectral Energy Distribution, Stellar Magnitude

Scientific paper

The eclipsing binary BW Dra has been observed during September 1980 and
May and June 1981 with a 48-inch reflector, using a two-beam multimode
nebular-stellar photometer with B- and V-filters. The star SAO 166029 is
taken as a point for comparison. Attention is presently given to the B-
and V-lightcurves obtained.

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