The evolved stellar system Sigma 2367

Details The evolved stellar system Sigma 2367 The evolved stellar system Sigma 2367

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982pasp...94..860b&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 94, Oct.-Nov. 1982, p. 860-871.

Astronomy and Astrophysics

Astronomy

6

Binary Stars, Orbital Elements, Stellar Evolution, Stellar Mass, Stellar Systems, Main Sequence Stars, Orbit Calculation, Radial Velocity, Star Clusters, Stellar Parallax, Stellar Spectra

Scientific paper

Visual and spectroscopic observations are employed to define the orbital elements of the binary Sigma 2367. The data were gathered with instrumentation at Cambridge, Mt. Palomar, and Victoria. A period of 33.528 days was determined for the binary system, with an absolute parallax of 0.0084 arcsec. The total mass of the two stars was set at 2.5 solar masses. A C component was identified as being physically related to the A and B components of the system.

Affiliated with

Also associated with

No associations

Rating

The evolved stellar system Sigma 2367 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 The evolved stellar system Sigma 2367, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The evolved stellar system Sigma 2367 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1032039