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Results 1 - 7 of 7
The formation history of the Milky Way disc with high-resolution cosmological simulations. (arXiv:2102.02652v1 [astro-ph.GA])
Volume 16, Issue 6 - article #10
M. Giammaria
,
A. Spagna
,
M. G. Lattanzi
,
G. Murante
,
P. Re Fiorentin
,
M. Valentini
http://arxiv.org/abs/2102.02652
An improved SPH scheme for cosmological simulations
Volume 10, Issue 8 - article #2
A.M. Beck
,
G. Murante
,
A. Arth
,
R.-S. Remus
,
A.F. Teklu
,
J.M.F. Donnert
,
S. Planelles
,
M.C. Beck
,
P. Foerster
,
M. Imgrund
,
K. Dolag
,
S. Borgani
arXiv.org - Astrophysics - Volume: 2015, Issue: 27 Feb
arXiv:1502.07358
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The thick disk rotation-metallicity correlation as a fossil of an “inverse chemical gradient” in the early Galaxy
Volume 7, Issue 51 - article #57
A. Curir
,
M. G. Lattanzi
,
A. Spagna
,
F. Matteucci
,
G. Murante
,
P. Re Fiorentin
and
E. Spitoni
Astronomy and Astrophysics - Volume: 545, Issue: September 2012
http://dx.doi.org/10.1051/0004-6361/201118558
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Simulating the evolution of disc galaxies in a group environment – I. The influence of the global tidal field
Volume 7, Issue 32 - article #15
Á. Villalobos
,
G. De Lucia
,
S. Borgani
and
G. Murante
Monthly Notices of the Royal Astronomical Society - Volume: 424, Issue: 4
Abstract
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The origin of abundance gradients in the Milky Way: the predictions of different models
Volume 4, Issue 12 - article #28
E. Colavitti
,
G. Cescutti
,
F. Matteucci
,
and
G. Murante
Astronomy and Astrophysics - Volume: 496, Issue: 2
Abstract
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PDF file (313.1 KB)
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PS file (249.5 KB)
The origin of abundance gradients in the Milky Way: the predictions of different models
Volume 3, Issue 48 - article #10
E. Colavitti
,
G. Cescutti
,
F. Matteucci
,
G. Murante
arXiv.org - Astrophysics - Volume: 2008, Issue: 27 Nov
arXiv:0811.3505
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The chemical evolution of a Milky Way-like galaxy: the importance of a cosmologically motivated infall law
Volume 3, Issue 19 - article #25
E. Colavitti
,
F. Matteucci
,
and
G. Murante
Astronomy and Astrophysics - Volume: 483, Issue: 2
Abstract
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Results 1 - 7 of 7
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