New observations of SS Cygni - Detection of total eclipses

Details New observations of SS Cygni - Detection of total eclipses New observations of SS Cygni - Detection of total eclipses

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70...61v&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 70, no. 1, p. 61-71.

Astronomy and Astrophysics

Astronomy

5

Accretion Disks, Astronomical Photometry, Dwarf Novae, Light Curve, Ubv Spectra, Eclipses, Starspots, Stellar Orbits

Scientific paper

New UBV photoelectric observations of the dwarf nova SS Cyg in quiescence are reported. Analysis of the entire present sample (1982-1991) made it possible to determine a photometrical period of 0.2751302 +/- 0.0000004 d, which coincides with the orbital one. The minimum at phi = 0.54 is absent in the middle of quiescence and appears before and immediately after the outburst. This definitely indicates an increase in the disk dimensions before the outburst - the hotspot is moving toward the star, giving rise to the conditions for a total eclipse.

Affiliated with

Also associated with

No associations

Rating

New observations of SS Cygni - Detection of total eclipses does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with New observations of SS Cygni - Detection of total eclipses, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and New observations of SS Cygni - Detection of total eclipses will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1273261