Photometry of the supersoft X-ray source V Sagittae during its large outburst in 2004

Details Photometry of the supersoft X-ray source V Sagittae during its large outburst in 2004 Photometry of the supersoft X-ray source V Sagittae during its large outburst in 2004

Feb 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006oejv...23...80s&link_type=abstract

Open European Journal on Variable Stars, Vol. 23, Proceedings of the 37th Conference on Variable Stars Research, Edited by L. Br

Computer Science

1

Scientific paper

New quadratic orbital elements of V Sge are presented. These was
computed using 14 minima timings obtained in 2004. During this
photometric campaing, the star was undergoing large outburst, which was
measured in detail using CCD.

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