scholarly journals THE CHEMICAL COMPOSITION OF RED GIANT STARS IN FOUR INTERMEDIATE-AGE CLUSTERS OF THE LARGE MAGELLANIC CLOUD

2008 ◽  
Vol 136 (1) ◽  
pp. 375-388 ◽  
Author(s):  
Alessio Mucciarelli ◽  
Eugenio Carretta ◽  
Livia Origlia ◽  
Francesco R. Ferraro
2006 ◽  
Vol 640 (2) ◽  
pp. 801-822 ◽  
Author(s):  
Jennifer A. Johnson ◽  
Inese I. Ivans ◽  
Peter B. Stetson

2006 ◽  
Vol 646 (2) ◽  
pp. 939-950 ◽  
Author(s):  
Alessio Mucciarelli ◽  
Livia Origlia ◽  
Francesco R. Ferraro ◽  
Claudia Maraston ◽  
Vincenzo Testa

2019 ◽  
Vol 488 (3) ◽  
pp. 3211-3221
Author(s):  
V Kovtyukh ◽  
B Lemasle ◽  
A Kniazev ◽  
L Berdnikov ◽  
G Bono ◽  
...  

Abstract We report the discovery of two new lithium-rich Cepheids in the Milky Way (A(Li) ≈ 2.9 dex) among the targets of the MAGIC spectroscopic survey with the Southern African Large Telescope spectrographs. The 6707 Å Li feature is usually not detectable in the atmosphere of Cepheids. Only three Cepheids (two in the Milky Way and one in the Large Magellanic Cloud) had been reported so far with high lithium abundances. We examine the possibility that the Li-rich Cepheids are evolving towards the red giant branch, crossing the instability strip for the first time, as well as other possible scenarios. The two stars are mixed-mode Cepheids pulsating simultaneously in the first and in the second overtone modes. We briefly discuss the possible connection between their unusual chemical composition and their pulsational properties.


2009 ◽  
Vol 5 (S268) ◽  
pp. 183-184 ◽  
Author(s):  
A. F. Marino ◽  
G. Piotto ◽  
R. Gratton ◽  
A. P. Milone ◽  
M. Zoccali ◽  
...  

AbstractWe derive abundances of Fe, Na, O, α and s-elements from GIRAFFE@VLT spectra for more than 200 red giant stars in the Milky Way satellite ω Centauri. Our preliminary results are that: (i) we confirm that ω Centauri exhibits large star-to-star metallicity variation (~1.4 dex); (ii) the metallicity distribution reveals the presence of at least five stellar populations with different [Fe/H]; (iii) a distinct Na-O anticorrelation is clearly observed for the metal-poor and metal-intermediate stellar populations while apparently the anticorrelation disappears for the most metal rich populations. Interestingly the Na level grows with iron.


1999 ◽  
Vol 190 ◽  
pp. 374-376
Author(s):  
Léo Girardi

We have developed a population synthesis code, aimed mainly at the interpretation of CMDs. Magellanic Cloud clusters have been largely used for the test/calibration of the underlying stellar tracks.


1998 ◽  
Vol 116 (2) ◽  
pp. 707-722 ◽  
Author(s):  
David B. Reitzel ◽  
Puragra Guhathakurta ◽  
Andrew Gould

2006 ◽  
Vol 650 (1) ◽  
pp. L55-L58 ◽  
Author(s):  
A. Derekas ◽  
L. L. Kiss ◽  
T. R. Bedding ◽  
H. Kjeldsen ◽  
P. Lah ◽  
...  

Icarus ◽  
1989 ◽  
Vol 81 (1) ◽  
pp. 24-30 ◽  
Author(s):  
John J. Matese ◽  
Daniel P. Whitmire ◽  
Ray T. Reynolds

2018 ◽  
Vol 861 (2) ◽  
pp. L16 ◽  
Author(s):  
Charlie Conroy ◽  
Ana Bonaca ◽  
Rohan P. Naidu ◽  
Daniel J. Eisenstein ◽  
Benjamin D. Johnson ◽  
...  

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