Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aj....112.1551b&link_type=abstract
Astronomical Journal v.112, p.1551
Astronomy and Astrophysics
Astronomy
43
Galaxy: Halo, Ism: Individual: Ngc 2112, Ism: Individual: Tombaugh 2, Ism: Individual: Melotte 71, Galaxy: Abundances
Scientific paper
We have analyzed high-dispersion echelle spectra of two or three stars each in the old anticenter disk clusters Tombaugh 2, NGC 2112, and Melotte 71. We find all three clusters to be mildly metal deficient, with [Fe/H]≃-0.45, -0.1, and -0.3, respectively, with an error of ˜0.2 dex. The clusters also have slight overdeficiencies of oxygen and nearly solar proportions of the α elements, indicating a lower relative contribution by massive stars to the chemical evolution of the outer Galactic disk. The clusters are found to be less metal deficient than photometric and low-resolution spectroscopic studies had indicated, which we attribute to severe nonmember contamination in those samples and/or reddening uncertainties. Our analysis suggests reddening values of E(B - V) =0.3-0.4 for Tom 2 and E(B - V) ≍0.6 for NGC 2112. NGC 2112 suffers from severe field star contamination.
Brown Jeffery A.
Geisler Doug
Oke Bev J.
Wallerstein George
No associations
LandOfFree
Chemical abundances in the Outer Disk Clusters Tombaugh 2, Melotte 71, and NGC 2112 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 Chemical abundances in the Outer Disk Clusters Tombaugh 2, Melotte 71, and NGC 2112, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Chemical abundances in the Outer Disk Clusters Tombaugh 2, Melotte 71, and NGC 2112 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1212219