FORS2/VLT survey of Milky Way globular clusters: II. Fe and Mg abundances of 51 Milky Way globular clusters on a homogeneous scale

被引：0

作者：

Dias, B. ^{[1
,2
,3
]}

Barbuy, B. ^{[2
]}

Saviane, I. ^{[1
]}

Held, E.V. ^{[4
]}

Da Costa, G.S. ^{[5
]}

Ortolani, S. ^{[4
,6
]}

Gullieuszik, M. ^{[4
]}

Vásquez, S. ^{[7
,8
,9
]}

机构：

[1] European Southern Observatory, Alonso de Córdova 3107, Santiago, Chile

[2] Universidade de São Paulo, Dept. de Astronomia, Rua do Matão 1226, São Paulo,05508-090, Brazil

[3] Department of Physics, Durham University, South Road, Durham,DH1 3LE, United Kingdom

[4] INAF, Osservatorio Astronomico di Padova, Vicolo dell'Osservatorio 5, Padova,35122, Italy

[5] Research School of Astronomy and Astrophysics, Australian National University, Mount Stromlo Observatory, via Cotter Road, Weston Creek,ACT,2611, Australia

[6] Università di Padova, Dipartimento di Astronomia, Vicolo dell'Osservatorio 2, Padova,35122, Italy

[7] Instituto de Astrofísica, Pontificia Universidad Católica de Chile, Av. Vicuña Mackenna 4860, Macul,Santiago,782-0436, Chile

[8] Millennium Institute of Astrophysics, Av. Vicuña Mackenna 4860, Macul,Santiago,782-0436, Chile

[9] Museo Interactivo Mirador, Dirección de Educación, Av. Punta Arenas, La Granja,Santiago,6711, Chile

来源：

Astronomy and Astrophysics | 2016年 / 590卷

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