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Results 1 - 10 of 10
Chemical evolution with rotating massive star yields II. A new assessment of the solar s- and r- process components. (arXiv:1911.02545v1 [astro-ph.GA])
Volume 14, Issue 45 - article #1
N. Prantzos
,
C. Abia
,
S. Cristallo
,
M. Limongi
,
A. Chieffi
http://arxiv.org/abs/1911.02545
The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young field stars. (arXiv:1703.00762v1 [astro-ph.GA])
Volume 12, Issue 9 - article #12
L. Magrini
,
S. Randich
,
G. Kordopatis
,
N. Prantzos
,
D. Romano
,
A. Chieffi
,
M. Limongi
,
P. Francois
,
E. Pancino
,
E. Friel
,
A. Bragaglia
,
G. Tautvaivsiene
,
L. Spina
,
J. Overbeek
,
T. Cantat-Gaudin
,
P. Donati
,
A. Vallenari
,
R. Sordo
,
F. M. Jimenez-Esteban
,
B. Tang
,
A. Drazdauskas
,
S. Sousa
,
S. Duffau
,
P. Jofre
,
G. Gilmore
,
S. Feltzing
,
E. Alfaro
,
T. Bensby
,
E. Flaccomio
,
S. Koposov
,
A. Lanzafame
,
R. Smiljanic
,
A. Bayo
,
G. Carraro
,
A. R. Casey
,
M. T. Costado
,
F. Damiani
,
E. Franciosini
,
A. Hourihane
,
C. Lardo
,
J. Lewis
,
L. Monaco
,
L. Morbidelli
,
G. Sacco
,
L. Sbordone
,
C.C. Worley
,
S. Zaggia
http://arxiv.org/abs/1703.00762
Dust grains from the heart of supernovae
Volume 11, Issue 5 - article #2
M. Bocchio
,
S. Marassi
,
R. Schneider
,
S. Bianchi
,
M. Limongi
,
A. Chieffi
arXiv.org - Astrophysics - Volume: 2016, Issue: 29 Jan
arXiv:1601.06770
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The metal and dust yields of the first massive stars
Volume 10, Issue 36 - article #12
S. Marassi
,
R. Schneider
,
M. Limongi
,
A. Chieffi
,
M. Bocchio
,
S. Bianchi
arXiv.org - Astrophysics - Volume: 2015, Issue: 2 Oct
arXiv:1509.08923
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TOPoS: II. On the bimodality of carbon abundance in CEMP stars. Implications on the early chemical evolution of galaxies
Volume 10, Issue 16 - article #19
P. Bonifacio
(1),
E. Caffau
(1,2),
M. Spite
(2),
M. Limongi
(3,4),
A. Chieffi
(5),
R.S. Klessen
(6,7,8),
P. François
(1,9),
P. Molaro
(10),
H. G. Ludwig
(2,1),
S. Zaggia
(11),
F. Spite
(1),
B. Plez
(12),
R. Cayrel
(1),
N. Christlieb
(2),
P.C. Clark
(13,6),
S.C.O. Glover
(6),
F. Hammer
(1),
A. Koch
(2),
L. Monaco
(14,15),
L. Sbordone
(16,17),
M. Steffen
(18,1)
((1) GEPI, Observatoire de Paris,
(2) ZAH-LSW,
(3) INAF - OA Roma,
(4) Kavli IPMU, Univ. Tokyo
(5) INAF - IASFC,
(6) ZAH-ARI,
(7) Kavli, IPAC, Stanford Univ.,
(8) Dep A&A Univ, Calfornia,
(9) UPJV, Univ. Picardie,
(10) INAF - OA Trieste,
(11) INAF- OA Padova,
(12) LUPM, Univ. Montpellier,
(13) School of Physics and Astronomy, Cardiff Univ.
(14) ESO,
(15) DCF - Univ. A. Bello,
(16) MAS,
(17) PUC - Chile,
(18) Leibniz-Institut AIP)
arXiv.org - Astrophysics - Volume: 2015, Issue: 24 Apr
arXiv:1504.05963
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The Origin of the Most Iron-poor Star
Volume 9, Issue 23 - article #72
S. Marassi
,
G. Chiaki
,
R. Schneider
,
M. Limongi
,
K. Omukai
,
T. Nozawa
,
A. Chieffi
,
and
N. Yoshida
The Astrophysical Journal - Volume: 794, Issue: 2
View article
PDF (638 KB)
Presupernova evolution and explosive nucleosynthesis of zero metal massive stars
Volume 7, Issue 8 - article #7
M. Limongi
,
A. Chieffi
arXiv.org - Astrophysics - Volume: 2012, Issue: 24 Feb
arXiv:1202.4581
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Sulfur in the globular clusters 47 Tucanae and NGC 6752
Volume 4, Issue 34 - article #33
L. Sbordone
,
M. Limongi
,
A. Chieffi
,
E. Caffau
,
H.-G. Ludwig
,
and
P. Bonifacio
Astronomy and Astrophysics - Volume: 503, Issue: 1
Abstract
|
PDF file (352.3 KB)
|
PS file (224.7 KB)
Sulphur in the Globular Clusters 47 Tucanae and NGC 6752
Volume 4, Issue 15 - article #10
L. Sbordone
,
M. Limongi
,
A. Chieffi
,
E. Caffau
,
H.-G. Ludwig
,
P. Bonifacio
arXiv.org - Astrophysics - Volume: 2009, Issue: 10 Apr
arXiv:0904.1417
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The chemical evolution of Omega Centauri's progenitor system
Volume 2, Issue 2 - article #14
D. Romano
(1),
F. Matteucci
(2),
M. Tosi
(1),
E. Pancino
(1),
M. Bellazzini
(1),
F. R. Ferraro
(3),
M. Limongi
(4),
A. Sollima
(3)
((1) INAF, Osservatorio Astronomico di Bologna;
(2) Dipartimento di Astronomia, Univ. di Trieste;
(3) Dipartimento di Astronomia, Univ. di Bologna;
(4) INAF, Osservatorio Astronomico di Roma)
ArXiv - Astrophysics
astro-ph/0701162 [
abs
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other
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Results 1 - 10 of 10
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