Physical parameters of solar neighbourhood flare stars

Details Physical parameters of solar neighbourhood flare stars Physical parameters of solar neighbourhood flare stars

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....82...53p&link_type=abstract

Astronomy and Astrophysics, vol. 82, no. 1-2, Feb. 1980, p. 53-60.

Astronomy and Astrophysics

Astrophysics

84

Flare Stars, Radii, Stellar Evolution, Stellar Luminosity, Stellar Spectrophotometry, Stellar Temperature, Binary Stars, Black Body Radiation, Data Processing, Electrophotometry, Stellar Magnitude

Scientific paper

Effective temperature, bolometric luminosity, and radius are estimated for 36 solar neighborhood flare stars from photoelectrically determined magnitudes by comparing the observed flux distributions to black body radiation. A comparison between the physical parameters derived from the observational data and theoretical models for low mass stars shows that solar neighborhood flare stars are situated on or close to the main sequence. The models of Grossman et al. (1974) are found to agree very well with observations. Radii obtained from the Barnes-Evans relation are compared to radii in the present work.

Affiliated with

Also associated with

No associations

Rating

Physical parameters of solar neighbourhood flare stars 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 Physical parameters of solar neighbourhood flare stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Physical parameters of solar neighbourhood flare stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1620102