The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248-Reference-Cited by-同舟云学术

The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248

Published:2002-06-20 Issue:2 Volume:572 Page:861-879
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Cowan John J.,Sneden Christopher,Burles Scott,Ivans Inese I.,Beers Timothy C.,Truran James W.,Lawler James E.,Primas Francesca,Fuller George M.,Pfeiffer Bernd,Kratz Karl‐Ludwig

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/572/i=2/a=861/pdf

Reference123 articles.

1. Broad-band $JHK(L')$ photometry of a sample of giants with 0.5 $\mathsf{>}$ [Fe/H] $\mathsf{>}$ -3

2. The effective temperature scale of giant stars (F0–K5)

3. Erratum The effective temperature scale of giant stars (F0-K5)

4. Reddening estimation for halo red giants using UVBY photometry

5. Ca [CSC]ii[/CSC] H and K Photometry on the [ITAL]uvby[/ITAL] System. III. The Metallicity Calibration for the Red Giants

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