EV Aurigae: A UU Herculis Star?

Details EV Aurigae: A UU Herculis Star? EV Aurigae: A UU Herculis Star?

Nov 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aps..ses..cb08y&link_type=abstract

American Physical Society, Southeastern Section Meeting, November 14-16, 1996, abstract #CB.08

Physics

Scientific paper

EV Aurigae was originally classified as a delta Cephei variable in 1943, with a period of 4.87228 days. Surprisingly, Berdnikov found no variability at all in 1985. CCD observations at VMI show some periodicity at up to 0.2 magnitude, but with a variable amplitude. We conclude that EV Aur may be a double-mode semi-regular variable, similar to the UU Her stars.

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