Spectroscopic Criteria for Isolating Members of Young Kinematic Groups in the Solar Neighborhood

Details Spectroscopic Criteria for Isolating Members of Young Kinematic Groups in the Solar Neighborhood Spectroscopic Criteria for Isolating Members of Young Kinematic Groups in the Solar Neighborhood

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..295s&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

This paper discusses spectroscopic age criteria for the true membership
of stars in young stellar groups, when the candidates were first
selected for purely kinematical reasons. The method is exemplified for
the cases of the Sirius group in UMa and the Pleiades.

Affiliated with

Also associated with

No associations

Rating

Spectroscopic Criteria for Isolating Members of Young Kinematic Groups in the Solar Neighborhood 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 Criteria for Isolating Members of Young Kinematic Groups in the Solar Neighborhood, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectroscopic Criteria for Isolating Members of Young Kinematic Groups in the Solar Neighborhood will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1508840