Metallicity of bulge clump giants in Baade's window (Hill+, 2011)

Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Stars: Giant, Abundances: [Fe/H], Photometry: Ubvri, Photometry: Infrared

Scientific paper

Stellar parameters and [Fe/H] and [Mg/H] abundances (and associated uncertainties) are given for a sample of 220 red clump stars selected in Baade's Window towards the Galactic Bulge and observed at a resolution of R=20,000 with the FLAMES/VLT multi-object spectrograph. The cross-identified UBVI (OGLE) and JHK (2MASS) photometry used for initial stellar parameter determination are also given.
(3 data files).

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Metallicity of bulge clump giants in Baade's window (Hill+, 2011) 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 Metallicity of bulge clump giants in Baade's window (Hill+, 2011), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Metallicity of bulge clump giants in Baade's window (Hill+, 2011) will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1671407

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.