We know that environment has a critical impact on galaxy growth and evolution. What we do not know is when it starts to have an impact and how it does it. I present results of our on-going survey of low surface brightness emission of cold molecular gas in protoclusters galaxies and their halos with the Australian Telescope Compact Array (ATCA). These findings alter our view of the important topics of the development and gas phase distribution of the "proto-intracluster medium": how ram pressure stripping may operate in protoclusters, how the galaxies may contribute to the proto-intracluster medium and how their star formation may be limited by dynamics. Finally, I present our new ATCA Large Program, COALAS (CO ATCA Legacy Archive of Star-Fo...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
<p>We know that environment has a critical impact on galaxy growth and evolution. What we do not kno...
It is clear that galaxies in local clusters are different from those in the field. Environment must ...
We know that environment has a critical impact on galaxy growth and evolution. What we do not know i...
International audienceIt is not yet known if the properties of molecular gas in distant protocluster...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
The formation and evolution of galaxies is fundamentally driven by the formation of new stars out of...
We report a detailed CO(1-0) survey of a galaxy protocluster field at z = 2.16, based on 475 h of ob...
The formation and evolution of galaxies is fundamentally driven by the formation of new stars out of...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
<p>We know that environment has a critical impact on galaxy growth and evolution. What we do not kno...
It is clear that galaxies in local clusters are different from those in the field. Environment must ...
We know that environment has a critical impact on galaxy growth and evolution. What we do not know i...
International audienceIt is not yet known if the properties of molecular gas in distant protocluster...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
It is not yet known if the properties of molecular gas in distant protocluster galaxies are signific...
The formation and evolution of galaxies is fundamentally driven by the formation of new stars out of...
We report a detailed CO(1-0) survey of a galaxy protocluster field at z = 2.16, based on 475 h of ob...
The formation and evolution of galaxies is fundamentally driven by the formation of new stars out of...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...
This paper presents the results of 475 hours of interferometric observations with the Australia Tele...