| |
Serna, A. |
| Volume |
Paper Title |
Page Number |
Authors |
| 94 |
Can the Dark Matter be Fully Baryonic? |
375 |
Alimi, J.-M.; Serna, A. |
| 390 |
Downsizing in Elliptical Galaxies: Some Clues from Self-consistent Hydrodynamical Simulations |
468 |
Domínguez-Tenreiro, R.; Oñorbe, J.; Serna, A.; González-García, A.C. |
| 390 |
The Luminous Matter Profiles in Ellipticals since z ∼ 1.5: The Photometric Plane and its Evolution |
498 |
Oñorbe, J.; Domínguez-Tenreiro, R.; Serna, A. |
| 421 |
Isolated Galaxies vs Galaxies in Groups: a Study of Their Properties from Cosmological Simulations |
241 |
Alpresa, P.; Onorbe, J.; Domínguez-Tenreiro, R.; Martínez-Serrano, F.; Serna, A. |
| 421 |
The Role of Gravitational Shock Heating in Isolated Galaxies from Cosmological Simulations |
275 |
Onorbe, J.; Dominguez-Tenreiro, R.; Martinez-Serrano, F. J.; Serna, A. |
| 421 |
The Origin of Massive Galaxies in Groups and Isolated: Law and Chance from Cosmological Simulations |
201 |
Domínguez-Tenreiro, R.; Alpresa, P.; Onorbe, J.; Martínez-Serrano, F.; Serna, A. |
| 453 |
Classical Bulge Formation with P-DEVA, a Chemodynamical AP3M-SPH Code |
371 |
Obreja, A.; Domínguez-Tenreiro, R.; Martínez-Serrano, F.; Doménech-Moral, M.; Serna, A. |
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