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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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1Publicado 2010“...≃ 1015 h-1 M⊙, over 50 per cent of satellite galaxies have experienced ram pressures ~10-11 h-2 dyn cm-2...”
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2Publicado 2006“... metals out of the galaxies. The asymptotically unbound baryon fraction drops from >95 per cent to ∼30...”
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3“... metals out of the galaxies. The asymptotically unbound baryon fraction drops from >95 per cent to ∼30...”
JOUR -
4“...≃ 1015 h-1 M⊙, over 50 per cent of satellite galaxies have experienced ram pressures ~10-11 h-2 dyn cm-2...”
JOUR -
5Publicado 2011“... contribution (∼15 per cent) from satellites that are accreted on nearly coplanar orbits. The inner regions...”
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6Publicado 2009“... satellite systems. Only ≈12 per cent of our model galaxies experienced a major merger during their lifetime...”
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7“... contribution (∼15 per cent) from satellites that are accreted on nearly coplanar orbits. The inner regions...”
JOUR -
8Publicado 2012“... in situ and with low α-enhancement from gas which never participated in a galactic outflow. Up to 15per...”
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9“... in situ and with low α-enhancement from gas which never participated in a galactic outflow. Up to 15per...”
JOUR -
10“... satellite systems. Only ≈12 per cent of our model galaxies experienced a major merger during their lifetime...”
JOUR -
11Publicado 2009“..., stellar masses and local densities diminishes the selection biases by ≈70 per cent. Based...”
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12“..., stellar masses and local densities diminishes the selection biases by ≈70 per cent. Based...”
JOUR -
13Publicado 2002“... of the stellar population in bulges at intermediate z with, at least, 50 per cent of the stars (in SCDM) being...”
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14Publicado 2007“... than 50 per cent of their stars at z ≥ 2, showing very weak evolution since this epoch. We also found...”
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15“... of the stellar population in bulges at intermediate z with, at least, 50 per cent of the stars (in SCDM) being...”
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16Publicado 2009“... per cent of its total stellar mass. Four of the eight galaxies nevertheless have well-formed disc...”
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17Publicado 2005“... of metal-dependent cooling produces 25 per cent more stars outside the central region than simulations...”
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18Publicado 2007“... formation activity. Nevertheless, this process accounts only for a ̃10 per cent increase of the fraction...”
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19Publicado 2003“... to unveil the effects of having a close companion. We found that about 50 per cent of GPs do not show signs...”
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20“... than 50 per cent of their stars at z ≥ 2, showing very weak evolution since this epoch. We also found...”
JOUR