Astronomy and Astrophysics – Astrophysics
Scientific paper
1996-11-26
Astron.J.113:806-822,1997
Astronomy and Astrophysics
Astrophysics
AASTeX, 43 pages, 11 figures, A.J. accepted
Scientific paper
10.1086/118302
We present a spectroscopic classification system for M-dwarfs and M-subdwarfs based on quantitative measures of TiO and CaH features in the region 6200 - 7400 Angstroms. Our sample of cool stars covers the range from solar metallicity stars to the most extreme subdwarfs known. Using synthetic spectra computed by Allard and Hauschildt (1995), we derive metallicities for the stars. Stars are classified as dwarfs (M V), subdwarfs (sdM), or extreme subdwarfs (esdM). These classifications correspond to [m/H] ~ 0.0, -1.2, and -2.0 respectively. Our metallicity scale agrees with theoretical HR diagrams and HST globular cluster measurements. We discuss some nearby subdwarfs of particular interest in light of our metallicity scale.
No associations
LandOfFree
M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale 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 M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and M-Subdwarfs: Spectroscopic Classification and the Metallicity Scale will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-515326