Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members-Reference-Cited by-同舟云学术

Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members

Published:2012-07 Issue: Volume:543 Page:A106
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Brogaard K.,VandenBerg D. A.,Bruntt H.,Grundahl F.,Frandsen S.,Bedin L. R.,Milone A. P.,Dotter A.,Feiden G. A.,Stetson P. B.,Sandquist E.,Miglio A.,Stello D.,Jessen-Hansen J.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361/201219196/pdf

Reference66 articles.

1. Accurate masses and radii of normal stars

2. vbyCaHβ CCD Photometry of Clusters. VIII. The Super-Metal-Rich, Old Open Cluster NGC 6791

3. WIYN OPEN CLUSTER STUDY. XXXIX. ABUNDANCES IN NGC 6253 FROM HYDRA SPECTROSCOPY OF THE Li 6708 Å REGION

4. The Chemical Composition of the Sun

5. SOUNDING OPEN CLUSTERS: ASTEROSEISMIC CONSTRAINTS FROM KEPLER ON THE PROPERTIES OF NGC 6791 AND NGC 6819

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