Radial velocity study of SS Cygni and RU Pegasi
Spectra of the two dwarf novae SS Cygni and RU Pegasi have been analyzed in a manner that is believed to reduce systematic errors arising from asymmetric mass motions. Revised spectroscopic orbital elements for the two systems are presented along with estimates of the component masses and orbital inclination of SS Cygni and limits to the component masses and orbital inclination of RU Pegasi.
- Research Organization:
- Department of Astronomy, University of Texas at Austin, Austin, Texas 78712
- OSTI ID:
- 6354079
- Journal Information:
- Astron. J.; (United States), Journal Name: Astron. J.; (United States) Vol. 84:5; ISSN ANJOA
- Country of Publication:
- United States
- Language:
- English
Similar Records
Time resolved spectroscopy of cataclysmic variables: SS Cygni
The quasi-coherent oscillations of SS Cygni
THE ACCRETING WHITE DWARF IN SS CYGNI REVEALED
Journal Article
·
Mon Sep 01 00:00:00 EDT 1980
· Astrophys. J.; (United States)
·
OSTI ID:6660478
The quasi-coherent oscillations of SS Cygni
Conference
·
Thu Aug 01 00:00:00 EDT 1996
·
OSTI ID:390468
THE ACCRETING WHITE DWARF IN SS CYGNI REVEALED
Journal Article
·
Sun Jun 20 00:00:00 EDT 2010
· Astrophysical Journal Letters
·
OSTI ID:21450948