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The evolution of the dust temperatures of galaxies in the SFR plane up to
B. Magnelli, D. Lutz, A. Saintonge +38
[Abridged] We study the evolution of the dust temperatures of galaxies in the SFR-M* plane up to z~2 using observations from the Herschel Space Observatory. Starting from a sample…
The suppression of star formation by powerful active galactic nuclei
M. J. Page, M. Symeonidis, J. D. Vieira +75
The old, red stars which constitute the bulges of galaxies, and the massive black holes at their centres, are the relics of a period in cosmic history when galaxies formed stars at…
Reversal or no reversal: the evolution of the star formation rate-density relation up to z~1.6
F. Ziparo, P. Popesso, A. Finoguenov +27
We investigate the evolution of the star formation rate (SFR)-density relation in the Extended Chandra Deep Field South (ECDFS) and the Great Observatories Origin Deep Survey (GOOD…
Mid- to far infrared properties of star-forming galaxies and active galactic nuclei
G. E. Magdis, D. Rigopoulou, G. Helou +19
We study the mid- to far-IR properties of a 24um-selected flux-limited sample (S24 > 5mJy) of 154 intermediate redshift (<z>~0.15), infrared luminous galaxies, drawn from the 5MUSE…
The long lives of giant clumps and the birth of outflows in gas-rich galaxies at high redshift
Frederic Bournaud, Valentin Perret, Florent Renaud +13
Star-forming disk galaxies at high redshift are often subject to violent disk instability, characterized by giant clumps whose fate is yet to be understood. The main question is wh…
The lack of star formation gradients in galaxy groups up to z~1.6
Felicia Ziparo, Paola Popesso, Andrea Biviano +28
In the local Universe, galaxy properties show a strong dependence on environment. In cluster cores, early type galaxies dominate, whereas star-forming galaxies are more and more co…