A radial velocity study of SS Cygni and RU Pegasi

Details A radial velocity study of SS Cygni and RU Pegasi A radial velocity study of SS Cygni and RU Pegasi

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979aj.....84..655k&link_type=abstract

Astronomical Journal, vol. 84, May 1979, p. 655-660.

Astronomy and Astrophysics

Astronomy

43

Binary Stars, Novae, Radial Velocity, Orbital Elements, Stellar Mass Accretion, Tables (Data), Velocity Distribution, White Dwarf Stars

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

A radial velocity study of SS Cygni and RU Pegasi 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 A radial velocity study of SS Cygni and RU Pegasi, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A radial velocity study of SS Cygni and RU Pegasi will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1701736