Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..219v&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Mar. 1986, p. 219-228) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Mar.-Apr
Astronomy and Astrophysics
Astronomy
8
Accretion Disks, Dwarf Novae, Light Curve, Stellar Flares, Stellar Spectrophotometry, Ubv Spectra, White Dwarf Stars
Scientific paper
New photoelectric photometry of SS Cyg during quiet states (minimum light) in 1983-1984 confirms the previous finding that partial eclipses are occurring in this binary system at epochs of conjunction. Orbital (6.6 h) UBV light curves are derived. Their shape depends on the phase of the approximately 51-d flare cycle, indicating that the system regularly experiences a stable state 25-15 d prior to a flare, followed by an unstable quiescent preflare state. Certain disparities between the orbital curves during the two phases may be attributable to preflare enlargement of the white dwarf accretion disk.
No associations
LandOfFree
UBV photometry of dwarf novae at minimum light. II - Preflare enlargement of the SS Cygni accretion disk 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 UBV photometry of dwarf novae at minimum light. II - Preflare enlargement of the SS Cygni accretion disk, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBV photometry of dwarf novae at minimum light. II - Preflare enlargement of the SS Cygni accretion disk will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1103581