The hottest horizontal-branch stars in ω Centauri. Late hot flasher vs. helium enrichment

被引：0

作者：

Moehler, S. ^{[1
]}

Dreizler, S. ^{[2
]}

Lanz, T. ^{[3
]}

Bono, G. ^{[4
]}

Sweigart, A.V. ^{[5
]}

Calamida, A. ^{[4
]}

Monelli, M. ^{[6
]}

Nonino, M. ^{[7
]}

机构：

[1] European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany

[2] Georg-August-Universität, Institut für Astrophysik, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany

[3] Department of Astronomy, University of Maryland, College Park, MD 20742-2421, United States

[4] INAF - Rome Astronomical Observatory, via Frascati 33, 00040 Monte Porzio Catone, Italy

[5] NASA Goddard Space Flight Center, Code 667, Greenbelt, MD 20771, United States

[6] IAC - Instituto de Astrofisica de Canarias, Calle via Lactea, 38200 La Laguna, Tenerife, Spain

[7] INAF - Trieste Astronomical Observatory, via G.B. Tiepolo 11, 40131 Trieste, Italy

来源：

Astronomy and Astrophysics | 2007年 / 475卷 / 02期

关键词：

Stars;

D O I：

暂无

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学科分类号：

摘要：

Journal article (JA)

引用

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