Photometric analysis of RR Lyrae stars

Details Photometric analysis of RR Lyrae stars Photometric analysis of RR Lyrae stars

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...209...59p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 209, no. 1-2, Jan. 1989, p. 59-66.

Astronomy and Astrophysics

Astrophysics

5

Astronomical Photometry, Stellar Oscillations, Ubv Spectra, Variable Stars, Horizontal Branch Stars, Light Curve, Lyra Constellation, Periodic Variations

Scientific paper

A UBV photometric analysis of the RRc type star ST CVn has been carried out. The results indicate that more than one frequency is present and the periods determined, 1.3236, 0.3290 and 0.1614 d explain the long term variation. Comparison of the derived physical parameters with theoretical models has also been carried out, indicating that these models are too cold for this star.

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