Photometric Evolution of the Orbital Light Curves of the Slow Nova V723 Cas

Details Photometric Evolution of the Orbital Light Curves of the Slow Nova V723 Cas Photometric Evolution of the Orbital Light Curves of the Slow Nova V723 Cas

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005ap%26ss.296..431s&link_type=abstract

Astrophysics and Space Science, Volume 296, Issue 1-4, pp. 431-434

Astronomy and Astrophysics

Astrophysics

1

Stars, Binaries, Novae, Photometry

Scientific paper

UBVRI photoelectric and CCD photometry of the slow nova V723 Cas obtained in the years 1995 2003 is presented. The evolution of light curves in 1-year intervals, folded with the orbital period 0.69326 days, shows an increase of the amplitude of the wave-like variations from 0.07 to 1.3 mag during the years 1997 2003. The fact that the shape and amplitude of the orbital light curves does not depend on wavelength is most probably related to the geometry of eclipses combined with the distribution of circumstellar matter in the system.

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