Mapping the Local Galactic Halo. I. Optical Photometry of Cool Subdwarf Candidates

Details Mapping the Local Galactic Halo. I. Optical Photometry of Cool Subdwarf Candidates Mapping the Local Galactic Halo. I. Optical Photometry of Cool Subdwarf Candidates

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aj....134..778m&link_type=abstract

The Astronomical Journal, Volume 134, Issue 2, pp. 778-786.

Astronomy and Astrophysics

Astronomy

3

Galaxy: Halo, Solar Neighborhood, Stars: Late-Type, Subdwarfs

Scientific paper

Optical (BVRI) photometric measurements of a sample of 564 candidate cool subdwarfs in the nearby halo are presented. The stars generally span the color range 0.4<(B-V)<1.8 hence, the sample is composed of early F- through early M-type stars on the subdwarf sequence. The sample is selected from the revised NLTT catalog of Gould and Salim and Salim and Gould via a reduced proper motion diagram. The photometry is precise and accurate; in particular, for stars with 9

Affiliated with

Also associated with

No associations

Rating

Mapping the Local Galactic Halo. I. Optical Photometry of Cool Subdwarf Candidates 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 Mapping the Local Galactic Halo. I. Optical Photometry of Cool Subdwarf Candidates, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mapping the Local Galactic Halo. I. Optical Photometry of Cool Subdwarf Candidates will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-958877