Materias dentro de su búsqueda.
Materias dentro de su búsqueda.
Galaxies: evolution
13
Galaxies: formation
11
Cosmology: theory
9
Galaxies: abundances
5
Galaxies: interactions
4
Methods: numerical
4
Evolution - galaxies
2
Galaxies
2
Galaxies: structure
2
Galaxy
2
Theory
2
Abundances - galaxies
1
Binaries
1
Cosmology
1
Dark Matter
1
Dark matter
1
Dark matter halos
1
Dark matter particles
1
Empirical model
1
Evolution-galaxies
1
Formation - cosmology
1
Formation-cosmology
1
Galaxies evolution
1
Galaxies formation
1
Galaxies haloes
1
Galaxies: bulges
1
Galaxies: clusters: general
1
Galaxies: clusters: intracluster medium
1
Galaxies: formation Galaxies: interactions
1
Galaxies: halos
1
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1“... progenitors. The model that better reproduces observations assumes that an ~20 per cent fraction of low...”
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2“... 80 per cent of its present mass within the virial radius. Furthermore, the mass accretion history...”
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3“... metals out of the galaxies. The asymptotically unbound baryon fraction drops from >95 per cent to ∼30...”
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4“...≃ 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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5“... contribution (∼15 per cent) from satellites that are accreted on nearly coplanar orbits. The inner regions...”
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6“... in situ and with low α-enhancement from gas which never participated in a galactic outflow. Up to 15per...”
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7“... satellite systems. Only ≈12 per cent of our model galaxies experienced a major merger during their lifetime...”
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8“... haloes possess an additional contribution from disc-heated stars, in the range ~3-30 per cent, with a...”
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9“... the decrease in its star formation activity. The fact that the fraction of ejected metals exceeds 60 per cent...”
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10“... profiles within residuals of ~10 per cent, in case the contribution from in situ stars remains small. Using...”
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11“..., the outer-halo populations contribute about 20-40 per cent in the fiducial solar neighbourhood...”
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12“... as the energy released per SN event is increased, with the consequent flattening of the bulge profile...”
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13“... 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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14“... 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“... per cent of galaxies above the demarcation line have a close companion or have experienced a recent...”
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16“... per cent of its total stellar mass. Four of the eight galaxies nevertheless have well-formed disc...”
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17“... of metal-dependent cooling produces 25 per cent more stars outside the central region than simulations...”
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18“... 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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19“... 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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20“.... We found that ~ 88 per cent of the observable host galaxies with mean gas metallicity lower than 0.6...”
JOUR