Color variations during activity states of the binary V Sge

Details Color variations during activity states of the binary V Sge Color variations during activity states of the binary V Sge

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..599..943s&link_type=abstract

X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. Edited by Nicholas E. White, Giuseppe Malaguti, and G

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Eclipsing Binaries, X-Ray Sources, X-Ray Bursts, Cataclysmic Binaries, Symbiotic Stars, Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables

Scientific paper

Color variations in V Sge during various states of its activity in the course of 1995-1997 show that B-V gets bluer while U-B does not change significantly. Comparison of our data with the outburst observed by Herbig et al. (1965) shows that although the character of the activity in V Sge changed during the last decades (Šimon and Mattei 1999) the colors and their variations remained similar. .

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