A Recent Photoelectric Minimum of RZ Cassiopeiae

Details A Recent Photoelectric Minimum of RZ Cassiopeiae A Recent Photoelectric Minimum of RZ Cassiopeiae

Jun 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972javso...1...54s&link_type=abstract

The Journal of the American Association of Variable Star Observers, vol. 1, no. 2, p. 54-55

Physics

2

Variables, Photoelectric Photometry, Tz Cas

Scientific paper

RZ Cassiopeiae (HD 17138 (A2); alpha= 2h 39m53s, delta= +69°13'
(1900) is an Algol type eclipsing binary star with a period of 1.195d.
Changes in its period in the past two decades have made it an
interesting object to observe for further possible changes.

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