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Evento Id: 406
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Dove: Rome
Data & Ora: 01-07-2012 10:00 (durata: 6 days)
Titolo: EWASS 2012 - Molecular gas in high redshift galaxies symposium at the European Week of Astronomy and Space Science
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Abstract:
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EWASS2012
Molecular gas in high redshift galaxies,  symposium at the
European Week of Astronomy and Space Science

EWASS 2012
1-6 July, 2012 Rome



Rationale

One of the outstanding questions in galaxy formation and evolution is how galaxies get their gas, and how that gas is transformed into stars over Cosmic Time. This research will undergo a major boost in the coming years, as greatly improved sensitivities of millimeter and radio facilities will be available. They will enable detailed investigations of the molecular content of high-z galaxies that are responsible for the bulk of the cosmic star formation and trace galaxy evolution out to the re-ionization epoch.

Recent observations are challenging our current understanding of galaxy formation, the emerging picture is that the evolution of the cosmic star formation rate density is largely driven by the evolution of the molecular gas content in galaxies. Studies of the complex multi-phase ISM of primeval galaxies are key to understanding the underlying physical processes. The greatly improved capabilities of existing submm-mm-radio observatories, as well as the advent of new facilities, is greatly enhancing the observational capabilities required for these studies and enable key measurements that were simply impossible so far.

This symposium will bring together experts in the field, reviewing  both the observational and the theoretical aspects of the molecular phase and of the ISM in high-z galaxies. The symposium is also expected to host many young scientists who will illustrate the most recent highlights obtained with the major facilities, such as ALMA, EVLA, IRAM, CARMA, APEX and Herschel.

The main topics to be covered by the proposed symposium are:
- molecular gas tracers as unbiased tools to detect and identify high-z galaxies;
- evolution of the molecular gas content through cosmic times;
- the star formation law and the modes of star formation at high redshift;
- structure, physics and dynamics of high-z galaxies inferred from molecular gas tracers;
- interplay between star formation and black hole accretion as inferred from molecular gas tracers.

These topics will be addressed both from an observational and a theoretical perspective, hence delivering the most comprehensive view of galaxy formation and evolution to date.


Abstract submission

Invited speakers

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Venue, Registration and Contacts


SOC
Carlos De Breuck, Roberto Maiolino (chair), Vernesa Smolcic, Linda Tacconi, Fabian Walter (co-chair) 
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Tipo di Evento: Congresso
Link: link
Presentazioni Disponibili:
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