Photometry of variable stars with periods near 1 day

Details Photometry of variable stars with periods near 1 day Photometry of variable stars with periods near 1 day

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.235.1059l&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 235, Dec. 15, 1988, p. 1059-1072.

Astronomy and Astrophysics

Astronomy

16

Astronomical Photometry, Variable Stars, Cepheid Variables, Light Curve, Metallicity, Milky Way Galaxy, Tables (Data)

Scientific paper

Accurate well-sampled light curves for seven short-period type-II Cepheid candidates are presented. It is demonstrated that CM UMa has a period of 0.589 and is an RRab star. The results show that CE Her and XX Vir are both type I Cepheids with excess scatter and rapid variations during declining light. BB Gem is found to be the shortest-period fundamental pulsator of the known Galactic classical Cepheids.

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