Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...128...37s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 128, no. 1, Nov. 1983, p. 37-52.
Astronomy and Astrophysics
Astronomy
41
Dwarf Novae, Eclipsing Binary Stars, Stellar Spectrophotometry, Variable Stars, Infrared Astronomy, Line Spectra, Radial Velocity, Stellar Color, Visible Spectrum
Scientific paper
Results of phase resolved spectroscopy and high speed photometry in wavelength bands between 4000 Å and 8000 Å are presented for the eclipsing dwarf nova OY Carinae in quiescent state. The authors discuss the following topics in detail: The structure of the disk during quiescence, the line formation therein and the influence of the disk rotation on the radial velocity curve. The characteristics of the mean orbital light curve and its implications for the structure of the outer disk and the light sources in the system. The variations of the eclipse parameters within short time scales and the eruption cycle and the consequences for the question of accretion in quiescence. The resulting system parameters with respect to different sets of determining equations.
Hartmann K.
Schoembs R.
No associations
LandOfFree
The eclipsing dwarf nova OY Carinae. II - Spectroscopy and photometry during quiescence 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 The eclipsing dwarf nova OY Carinae. II - Spectroscopy and photometry during quiescence, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The eclipsing dwarf nova OY Carinae. II - Spectroscopy and photometry during quiescence will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1483816