Search for Photometric Abundance Indices for M Dwarf Stars

Details Search for Photometric Abundance Indices for M Dwarf Stars Search for Photometric Abundance Indices for M Dwarf Stars

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982jkas...15...49l&link_type=abstract

Journal of the korean Astronomical Society, vol. 15, no.2, p. 49-58

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The UBVRIHKL magnitude on Johnson system and space motions of M dwarf stars have been collected. This sample of M stars have been distinguished on a purely kinematical basis; the one with e<1.15, young disk population, with 1.150.3 halo population. On the color-color diagrams and the old disk stars and color excess-orbital eccentricity diagrams, there is no distinction between the disk stars and the young disk stars. However (I-H) color could be used to distinguish halo stars from young and old disk standard the color excesses, delta(U-B), delta(B-V), delta(V-R), delta(H-K), delta(K-L), and delta(B-R) can be used as abundance indicators only for the halo stars. But these color excesses which are measures of blue excesses, are positive for the halo stars with smaller eccentricities and become negative for those with larger eccentricities.

Affiliated with

Also associated with

No associations

Rating

Search for Photometric Abundance Indices for M Dwarf 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 Search for Photometric Abundance Indices for M Dwarf Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Search for Photometric Abundance Indices for M Dwarf Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-929904