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Cited article:
M. Di Criscienzo, P. Ventura, F. D'Antona
A&A, 496 1 (2009) 223-227
Published online: 2009-01-30
This article has been cited by the following article(s):
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Astrophysics studies with the Trojan Horse Method
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The Astrophysical Journal 801 (2) 113 (2015)
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A detailed study of the main sequence of the globular cluster NGC 6397: can we derive constraints on the existence of multiple populations?
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The Pisa pre-main sequence tracks and isochrones
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ASTROPHYSICAL IMPACT OF THE UPDATED9Be(p,α)6Li AND10B(p,α)7Be REACTION RATES AS DEDUCED BY THM
L. Lamia, C. Spitaleri, E. Tognelli, et al.
The Astrophysical Journal 811 (2) 99 (2015)
DOI: 10.1088/0004-637X/811/2/99
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Star formation in the starburst cluster in NGC 3603
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Astrophysics and Space Science 340 (2) 263 (2012)
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Empirical tests of pre-main-sequence stellar evolution models with eclipsing binaries
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Water contents of Earth-mass planets around M dwarfs
Feng Tian and Shigeru Ida
Nature Geoscience 8 (3) 177 (2015)
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Diluting the material forming the second generation stars in globular clusters: the contribution by unevolved stars
R. G. Gratton and E. Carretta
Astronomy and Astrophysics 521 A54 (2010)
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