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Results 1 - 5 of 5
Limits on Population III star formation with the most iron-poor stars
Volume 11, Issue 50 - article #12
de Bennassuti
,
M.
,
Salvadori
,
S.
,
Schneider
,
R.
,
Valiante
,
R.
,
Omukai
,
K.
>Oxford University Press
http://mnras.oxfordjournals.org/cgi/content/short/465/1/926?rss=1
Limits on Pop III star formation with the most iron-poor stars. (arXiv:1610.05777v1 [astro-ph.GA])
Volume 11, Issue 43 - article #7
M. de Bennassuti
,
S. Salvadori
,
R. Schneider
,
R. Valiante
http://arxiv.org/abs/1610.05777
Carbon-enhanced metal-poor stars in different environments
Volume 11, Issue 40 - article #14
S. Salvadori
,
Ã. Skúladóttir
,
M. de Bennassuti
John Wiley & Sons, Inc.
http://onlinelibrary.wiley.com/resolve/doi?DOI=10.1002%2Fasna.201612402
Carbon-enhanced metal-poor stars in different environments
Volume 10, Issue 46 - article #7
Stefania Salvadori
,
Asa Skuladottir
,
Matteo de Bennassuti
arXiv.org - Astrophysics - Volume: 2015, Issue: 18 Dec
arXiv:1512.05506
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Decoding the stellar fossils of the dusty Milky Way progenitors
Volume 9, Issue 22 - article #31
Matteo de Bennassuti
(1 and 2),
Raffaella Schneider
(2),
Rosa Valiante
(2),
Stefania Salvadori
(3)
((1) Dipartimento di Fisica, Sapienza, Universita` di Roma, Piazzale Aldo Moro 5, 00185, Roma, Italy,
(2) INAF - Osservatorio Astronomico di Roma, Via di Frascati 33, 00040 Monte Porzio Catone, Italy,
(3) Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The Netherlands)
arXiv.org - Astrophysics - Volume: 2014, Issue: 26 Sep
arXiv:1409.5798
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Results 1 - 5 of 5
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