Abundance analysis of red clump stars in the old, inner disc, open cluster NGC 4337: a twin of NGC 752?
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361/201424443/pdf
Reference31 articles.
1. The effective temperature scale of giant stars (F0–K5)
2. Extended Strömgren Photoelectric Photometry in NGC 752
3. BV photographic and CCD photometry of IC 4651
4. LITHIUM IN THE INTERMEDIATE-AGE OPEN CLUSTER, NGC 3680
5. The first chemical abundance analysis of K giants in the inner Galactic disc
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1. A Comparison of the Chemical Composition of Main-sequence and Giant Stars in the Open Cluster NCC 752;The Astrophysical Journal;2019-06-18
2. Investigating dynamical properties of evolved Galactic open clusters;Astronomy & Astrophysics;2019-04
3. On the mass of the Galactic star cluster NGC 4337;Monthly Notices of the Royal Astronomical Society;2017-03-01
4. Galactic Structure in the Outer Disk: The Field in the Line of Sight to the Intermediate-Age open Cluster Tombaugh 1;The Astronomical Journal;2017-02-07
5. RADIAL VELOCITIES AND METALLICITIES OF RED GIANT STARS IN THE OLD OPEN CLUSTER NGC 7762;The Astronomical Journal;2016-12-07
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