Absolute Magnitudes of Several Peculiar Star Groups

Details Absolute Magnitudes of Several Peculiar Star Groups Absolute Magnitudes of Several Peculiar Star Groups

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997esasp.402..429j&link_type=abstract

Proceedings of the ESA Symposium `Hipparcos - Venice '97', 13-16 May, Venice, Italy, ESA SP-402 (July 1997), p. 429-432

Physics

1

Scientific paper

We present absolute magnitude estimates for a number of peculiar star groups, defined on the basis of their spectral characteristics: Subdwarfs OB, He-strong stars, He variables, A-type shell stars, lambda Bootis stars, Cool subdwarfs, Weak G-band stars, Subgiants CH, Barium stars. A series of numerical simulations is used for deriving systematic corrections to be applied to the derived M_V. These results are used to assess the location in the HR diagram of the stars, and, when the size of the group is statistically significant, the evolutionary status of the group.

Affiliated with

Also associated with

No associations

Rating

Absolute Magnitudes of Several Peculiar Star Groups 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 Absolute Magnitudes of Several Peculiar Star Groups, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Absolute Magnitudes of Several Peculiar Star Groups will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1879275