Constraints on the companion object to HD 114762

Details Constraints on the companion object to HD 114762 Constraints on the companion object to HD 114762

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...380l..35c&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 380, Oct. 10, 1991, p. L35-L38.

Other

53

Binary Stars, Brown Dwarf Stars, Companion Stars, Planetary Systems, Radial Velocity, Stellar Mass, Stellar Orbits

Scientific paper

The paper presents high-precision radial velocity observations of the candidate planetary system HD 114762. The data obtained confirm Latham et al.'s (1989) of the binary nature of the system. The new orbital solution gives an eccentricity of 0.38 compared with the Latham et al. value of 0.25, but otherwise it agrees well with the discovery orbit. The mass function for the system implies a companion object with Mc sin i(orb) = 0.011 solar mass.

Affiliated with

Also associated with

No associations

Rating

Constraints on the companion object to HD 114762 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 Constraints on the companion object to HD 114762, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraints on the companion object to HD 114762 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1875425