Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
Galaxies: formation
Galaxies: evolution
13
Cosmology: theory
11
Galaxies: abundances
5
Galaxies: interactions
4
Methods: numerical
3
Galaxies: clusters: general
2
Dark matter
1
Galaxies: clusters: intracluster medium
1
Galaxies: elliptical and lenticular, cD
1
Galaxies: groups: general
1
Galaxies: structure
1
Galaxy: abundances
1
Intergalactic medium
1
Methods: N-body simulations
1
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1“... metals out of the galaxies. The asymptotically unbound baryon fraction drops from >95 per cent to ∼30...”
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2“...≃ 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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3“... contribution (∼15 per cent) from satellites that are accreted on nearly coplanar orbits. The inner regions...”
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4“... in situ and with low α-enhancement from gas which never participated in a galactic outflow. Up to 15per...”
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5“... satellite systems. Only ≈12 per cent of our model galaxies experienced a major merger during their lifetime...”
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6“..., stellar masses and local densities diminishes the selection biases by ≈70 per cent. Based...”
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7“... 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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8“... than 50 per cent of their stars at z ≥ 2, showing very weak evolution since this epoch. We also found...”
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9“... per cent of its total stellar mass. Four of the eight galaxies nevertheless have well-formed disc...”
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10“... formation activity. Nevertheless, this process accounts only for a ̃10 per cent increase of the fraction...”
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11“... of metal-dependent cooling produces 25 per cent more stars outside the central region than simulations...”
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12“... 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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13“... 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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14“.... On the other hand, mergers contribute with a larger fraction of stellar mass (≈10-20 per cent...”
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