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Ciencias Astronómicas
Galaxies: formation
Galaxies: evolution
4
Galaxies: interactions
3
Galaxies: clusters: general
2
Cosmology: theory
1
Física
1
Galaxies: abundances
1
Galaxies: clusters: intracluster medium
1
Galaxies: elliptical and lenticular, cD
1
Galaxies: groups: general
1
Galaxies: individual: NGC 4649
1
Galaxies: kinematics and dynamics
1
Galaxies: star clusters
1
Globular clusters: general
1
Intergalactic medium
1
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1por 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 -
2“..., stellar masses and local densities diminishes the selection biases by ≈70 per cent. Based...”
Aportado por: SEDICI (UNLP)Articulo -
3por 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 -
4“... 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 -
5por 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