Photometry of yellow semi-regular variables - SS GEM

Details Photometry of yellow semi-regular variables - SS GEM Photometry of yellow semi-regular variables - SS GEM

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.181..203z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 181, no. 2, July 1991, p. 203-210.

Astronomy and Astrophysics

Astrophysics

10

Astronomical Photometry, Stellar Color, Variable Stars, Curve Fitting, Light Curve

Scientific paper

New photoelectric photometry of SS Gem is presented. The period analysis and light curve fits show that the formal period is the pulsation period and there is a strong harmonic. The period variation of SS Gem is found to be similar to that of AC Her. It is argued that being a Population I object, SS Gem is not a low-mass star in the post-AGB phase but an intermediate-mass variable related to classical Cepheids.

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