The period and photometry of BC Draconis

Details The period and photometry of BC Draconis The period and photometry of BC Draconis

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26as...47..541s&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 47, Mar. 1982, p. 541-545.

Astronomy and Astrophysics

Astrophysics

1

Light Curve, Stellar Spectrophotometry, Variable Stars, Visual Photometry, Cepheid Variables, Electrophotometry, Hertzsprung-Russell Diagram

Scientific paper

It is found that BC Draconis appears to be a normal RR Lyrae-type
variable, with a period of 0.719576 days, by BV photoelectric photometry
subjected to frequency analysis. V light and B-V color curves of the
variable are given, and an O-C diagram is constructed from the
Strohmeier and Knigge (1961) photographic maxima.

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