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1Publicado 2006“... metals out of the galaxies. The asymptotically unbound baryon fraction drops from >95 per cent to ∼30...”
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2“... metals out of the galaxies. The asymptotically unbound baryon fraction drops from >95 per cent to ∼30...”
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3Publicado 2011“... contribution (∼15 per cent) from satellites that are accreted on nearly coplanar orbits. The inner regions...”
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4Publicado 2009“... satellite systems. Only ≈12 per cent of our model galaxies experienced a major merger during their lifetime...”
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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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6Publicado 2012“... in situ and with low α-enhancement from gas which never participated in a galactic outflow. Up to 15per...”
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7“... in situ and with low α-enhancement from gas which never participated in a galactic outflow. Up to 15per...”
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8“... satellite systems. Only ≈12 per cent of our model galaxies experienced a major merger during their lifetime...”
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9Publicado 2009“..., stellar masses and local densities diminishes the selection biases by ≈70 per cent. Based...”
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10“..., stellar masses and local densities diminishes the selection biases by ≈70 per cent. Based...”
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11Publicado 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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12Publicado 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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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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14Publicado 2009“... per cent of its total stellar mass. Four of the eight galaxies nevertheless have well-formed disc...”
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15Publicado 2005“... of metal-dependent cooling produces 25 per cent more stars outside the central region than simulations...”
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16Publicado 2007“... formation activity. Nevertheless, this process accounts only for a ̃10 per cent increase of the fraction...”
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17Publicado 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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18“... than 50 per cent of their stars at z ≥ 2, showing very weak evolution since this epoch. We also found...”
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19“... per cent of its total stellar mass. Four of the eight galaxies nevertheless have well-formed disc...”
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20“... formation activity. Nevertheless, this process accounts only for a ̃10 per cent increase of the fraction...”
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