Spectroscopic orbits of three K dwarf stars (Tokovinin+ 1994)

Details Spectroscopic orbits of three K dwarf stars (Tokovinin+ 1994) Spectroscopic orbits of three K dwarf stars (Tokovinin+ 1994)

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ycat..32820831t&link_type=abstract

VizieR On-line Data Catalog: J/A+A/282/831. Originally published in: 1994A&A...282..831T

Computer Science

Binaries: Spectroscopic, Radial Velocities, Stars: K-Type

Scientific paper

The spectroscopic orbits of single-lined binary dwarfs HD 23439B, HD 237287 and HD 217580 are derived from the radial velocities measured with two correlation radial-velocity spectrometers: correlation radial velocity (CORAVEL) at the 1m Swiss telescope of Observatoire de Haute-Provence, and radial velocity meters (RVM) used on several telescopes. The mutual agreement of these two data sets is analyzed and found to be quite good. The estimated minimum mass of secondary component corresponds to that of M-type dwarf for the first 2 systems and is equal to 0.06 solar mass for HD 217580. (3 data files).

Affiliated with

Also associated with

No associations

Rating

Spectroscopic orbits of three K dwarf stars (Tokovinin+ 1994) 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 orbits of three K dwarf stars (Tokovinin+ 1994), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic orbits of three K dwarf stars (Tokovinin+ 1994) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1587769