Metallicities, Relative Ages, and Kinematics of Stellar Populations in ω Centauri-Reference-Cited by-同舟云学术

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Metallicities, Relative Ages, and Kinematics of Stellar Populations in ω Centauri

Published:2005-11-20 Issue:1 Volume:634 Page:332-343
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Sollima A.,Pancino E.,Ferraro F. R.,Bellazzini M.,Straniero O.,Pasquini L.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference62 articles.

1. Signatures of Convection in the Spectrum of Procyon: Fundamental Parameters and Iron Abundance

2. Anderson J. 2002, in ASP Conf. Ser. 265, Omega Centauri, a Unique Window into Astrophysics, ed. F. van Leeuwen, J. D. Hughes, & G. Piotto (San Francisco: ASP), 87

3. Metallicities for old stellar systems from CA II triplet strengths in member giants

4. Line formation in solar granulation

5. Centauri: The Population Puzzle Goes Deeper

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1. Spectroscopic and dynamic orbital analyses of metal‐poor and high proper‐motion stars: I. HD 8724 and HD 195633;Astronomische Nachrichten;2024-07

2. MgAl burning chain in ω Centauri;Astronomy & Astrophysics;2024-01

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4. Detecting axion dark matter through the radio signal from Omega Centauri;Physical Review D;2021-11-10

5. A stellar census in globular clusters with MUSE;Astronomy & Astrophysics;2021-09

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