| |
Puech, M. |
| Volume |
Paper Title |
Page Number |
Authors |
| 390 |
Disentangling Interacting Galaxy Pairs and Entangling Them Back |
186 |
Fuentes-Carrera, I.; Amram, P.; Balkowski, C.; Flores, H.; Puech, M.; Yang, Y.; Rosado, M.; Hernández-Toledo, H. |
| 390 |
The Origin of Star Formation since z = 1 |
268 |
Hammer, F.; Puech, M.; Yang, Y.B.; Flores, H. |
| 390 |
IMAGES I. Classification of Galaxy Kinematics since z = 1 |
502 |
Yang, Y.; Flores, H.; Hammer, F.; Neichel, B.; Puech, M.; Nesvadba, N. |
| 396 |
The Milky Way is an Exceptionally Quiet Galaxy: Implications for Spiral Formation |
287 |
Puech, M.; Hammer, F.; Chemin, L.; Flores, H.; Lehnert, M. |
| 419 |
The Chemical Evolution of Intermediate Mass Galaxies over the Last 8 Gyrs |
331 |
Rodrigues, M.; Hammer, F.; Flores, H.; Puech, M. |
| 421 |
The Evolution of the Tully-Fisher Relation over the Past 6 Gyr |
281 |
Puech, M.; Hammer, F.; Flores, H.; Rodrigues, M.; Delgado, R.; Yang, Y. |
| 421 |
Simulating Observations of Distant Galaxies with the E-ELT |
282 |
Puech, M.; Rosati, P.; Toft, S. |
|
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