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Galaxies: formation
Galaxies: evolution
30
Cosmology: theory
23
Galaxies: abundances
11
Galaxies: interactions
11
Galaxies: clusters: general
6
Methods: numerical
6
Ciencias Astronómicas
5
Galaxies: clusters: intracluster medium
3
Galaxies: elliptical and lenticular, cD
3
Galaxies: groups: general
3
Intergalactic medium
3
Dark matter
2
Galaxies: structure
2
Galaxy: abundances
2
Methods: N-body simulations
2
Física
1
Galaxies: individual: NGC 4649
1
Galaxies: kinematics and dynamics
1
Galaxies: star clusters
1
Globular clusters: general
1
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21“... per cent of its total stellar mass. Four of the eight galaxies nevertheless have well-formed disc...”
JOUR -
22“... formation activity. Nevertheless, this process accounts only for a ̃10 per cent increase of the fraction...”
JOUR -
23“... of metal-dependent cooling produces 25 per cent more stars outside the central region than simulations...”
JOUR -
24“... to unveil the effects of having a close companion. We found that about 50 per cent of GPs do not show signs...”
JOUR -
25Publicado 2011“... simulations with respectively 20 and 50 per cent of the disc in the form of gas. We find that the more gas...”
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26“... simulations with respectively 20 and 50 per cent of the disc in the form of gas. We find that the more gas...”
JOUR -
27Publicado 2011“.... On the other hand, mergers contribute with a larger fraction of stellar mass (≈10-20 per cent...”
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28“.... On the other hand, mergers contribute with a larger fraction of stellar mass (≈10-20 per cent...”
JOUR -
29por Tecce, Tomás E., Cora, Sofía Alejandra, Tissera, Patricia B., Abadi, Mario G., Lagos, Claudia del Pilar“...>vir</SUB>≃ 10<SUP>15</SUP> h<SUP>-1</SUP> M⊙, over 50 per cent of satellite galaxies have experienced...”
Publicado 2010
Aportado por: SEDICI (UNLP)Articulo -
30“..., stellar masses and local densities diminishes the selection biases by ≈70 per cent. Based...”
Aportado por: SEDICI (UNLP)Articulo -
31por Bridges, Terry, Gebhardt, Karl, Sharples, Ray, Faifer, Favio Raúl, Forte, Juan Carlos, Beasley, Michael A., Zepf, Stephen E., Forbes, Duncan A., Hanes, David A., Pierce, Michael“... find no rotation of the GC system, with an upper limit of ν/σ < 0.6 at a confidence level of 95 per...”
Publicado 2006
Aportado por: SEDICI (UNLP)Articulo -
32“... simulations with respectively 20 and 50 per cent of the disc in the form of gas. We find that the more gas...”
Aportado por: SEDICI (UNLP)Articulo -
33por Jiménez, Noelia, Cora, Sofía Alejandra, Bassino, Lilia Patricia, Tecce, Tomás E., Smith Castelli, Analía Viviana“... contribute with a larger fraction of stellar mass (≈10-20 per cent), but the metallicity of the accreted...”
Publicado 2011
Aportado por: SEDICI (UNLP)Articulo