On the reality of the spectroscopic orbit for R Aquarii

Details On the reality of the spectroscopic orbit for R Aquarii On the reality of the spectroscopic orbit for R Aquarii

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasp...87..269j&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 87, Apr. 1975, p. 269-271

Astronomy and Astrophysics

Astronomy

18

Binary Stars, Line Spectra, Radial Velocity, Stellar Mass, Stellar Spectrophotometry, Variable Stars, Astronomical Spectroscopy, Emission Spectra, Stellar Mass Ejection, Stellar Spectra

Scientific paper

New velocities for the emission lines in R Aqr show that the system has
not followed the orbit with a period of 26.7 years tentatively suggested
by Merrill. The binary nature of the star and its enormous mass function
of 16.5 solar masses are probably unreal. Evidence for mass loss with
ionization and velocity increasing outward is presented.

Affiliated with

Also associated with

No associations

Rating

On the reality of the spectroscopic orbit for R Aquarii 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 On the reality of the spectroscopic orbit for R Aquarii, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the reality of the spectroscopic orbit for R Aquarii will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-948894