Context. Globular clusters are known to host multiple stellar populations, which are a signature of their formation process. The globular cluster E3 is one of the few low-mass globulars that is thought not to host multiple populations. Aims. We investigate red giant branch stars in E3 with the ai...
Monaco, L.
,
Villanova, S.
,
Carraro, G.
,
Mucciarelli, A.
,
Moni Bidin, C.
,
[Chemical abundance analysis of red giant branch stars in the globular cluster E3]
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Chemical abundance analysis of red giant branch stars in the globular cluster E3
We present Li, Na, Al, and Fe abundances of 199 lower red giant branch star members of the stellar system Omega Centauri, using high-resolution spectra acquired with FLAMES at the Very Large Telescope. The A(Li) distribution is peaked at A(Li) ∼ 1 dex with a prominent tail towards lower values. T...
Mucciarelli, A.
,
Salaris, M.
,
Monaco, L.
,
Bonifacio, P.
,
Fu, X.
,
Villanova, S.
,
[Lithium abundance in lower red giant branch stars of Omega Centauri]
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Lithium abundance in lower red giant branch stars of Omega Centauri
Aims. The aim of this work is the study of abundances of the heavy elements Ba, La, Ce, Nd, and Eu in 56 bulge giants (red giant branch and red clump) with metallicities ranging from 1 : 3 dex to 0 : 5 dex.
Methods. We obtained high-resolution spectra of our giant stars using the FLAMES-UVES sp...
Van der Swaelmen, M
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Barbuy, B
,
Hill, V
,
Zoccali, M
,
Minniti, D
,
Ortolani, S
,
Gomez, A
,
[Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants]
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Heavy elements Ba, La, Ce, Nd, and Eu in 56 Galactic bulge red giants