Oxygen abundances in metal-poor stars from IR OH lines

Details Oxygen abundances in metal-poor stars from IR OH lines Oxygen abundances in metal-poor stars from IR OH lines

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001newar..45..551m&link_type=abstract

New Astronomy Reviews, Volume 45, Issue 8, p. 551-553.

Astronomy and Astrophysics

Astronomy

2

Scientific paper

High-resolution spectra in the H-band (1.55-1.56 μm) were obtained with the Phoenix spectrograph at the 2.1 m Kitt Peak telescope, for the observation of OH lines in 14 metal-poor stars of metallicities -0.8<[Fe/H]<-2.2. Results of [O/Fe]~+0.43 are in agreement with oxygen-to-iron ratios derived from the forbidden [O I] lines, and in disagreement with the high [O/Fe] derived from permitted O I lines and recent determinations from UV OH lines.

Affiliated with

Also associated with

No associations

Rating

Oxygen abundances in metal-poor stars from IR OH lines 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 Oxygen abundances in metal-poor stars from IR OH lines, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Oxygen abundances in metal-poor stars from IR OH lines will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1204964