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Cited article:

Does the chemical signature of TYC 8442–1036–1 originate from a rotating massive star that died in a faint explosion?

G. Cescutti, M. Valentini, P. François, C. Chiappini, E. Depagne, N. Christlieb, C. Cortés

A&A, 595 (2016) A91

Published online: 2016-11-03

DOI: https://doi.org/10.1051/0004-6361/201629106

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Manganese spread in Ursa Minor as a proof of sub-classes of type Ia supernovae

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The CEMP star SDSS J0222–0313: the first evidence of proton ingestion in very low-metallicity AGB stars?

E. Caffau, L. Monaco, P. Bonifacio, et al.
Astronomy & Astrophysics 628 A46 (2019)
DOI: 10.1051/0004-6361/201935680
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Uncertainties in s-process nucleosynthesis in low-mass stars determined from Monte Carlo variations

G Cescutti, R Hirschi, N Nishimura, et al.
Monthly Notices of the Royal Astronomical Society 478 (3) 4101 (2018)
DOI: 10.1093/mnras/sty1185
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The oldest stars of the bulge: new information on the ancient Galaxy

Gabriele Cescutti, Cristina Chiappini and Raphael Hirschi
Proceedings of the International Astronomical Union 13 (S334) 94 (2017)
DOI: 10.1017/S1743921317008183
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