Spectroscopic binary orbits from photoelectric radial velocities. Paper 58: HR 1105

Details Spectroscopic binary orbits from photoelectric radial velocities. Paper 58: HR 1105 Spectroscopic binary orbits from photoelectric radial velocities. Paper 58: HR 1105

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984obs...104..224g&link_type=abstract

The Observatory, vol. 104, p. 224-231 (1984)

Physics

26

Scientific paper

The nature and causes of S-type spectra are reviewed. The S star HR 1105 is shown to be a spectroscopic binary with a period of 596 days. It is the first binary of type S to have its orbit determined, notwithstanding that it is arguably the brightest S star and that the variability of its velocity has been known since 1922, the same year as type S was recognized.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic binary orbits from photoelectric radial velocities. Paper 58: HR 1105 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 Spectroscopic binary orbits from photoelectric radial velocities. Paper 58: HR 1105, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic binary orbits from photoelectric radial velocities. Paper 58: HR 1105 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1229682