Luminosity Function of Field Stars with 0.85< B-V< 1.10

Details Luminosity Function of Field Stars with 0.85< B-V< 1.10 Luminosity Function of Field Stars with 0.85< B-V< 1.10

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..133h&link_type=abstract

The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ

Physics

Scientific paper

The color range 0m.85 < B-V < 1m.10 lies in the area of maximum concentration of evolved stars, so it is very difficult to identify low-proper-motion dwarfs of the same color. This paper discusses problems of differentiating between the spectral characteristics of subgiants and dwarfs in this color range. Implications for catalogues of nearby G and K dwarfs are analysed.

Affiliated with

Also associated with

No associations

Rating

Luminosity Function of Field Stars with 0.85< B-V< 1.10 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 Luminosity Function of Field Stars with 0.85< B-V< 1.10, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminosity Function of Field Stars with 0.85< B-V< 1.10 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1508813