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VIALACTEA - The Milky Way as a Star Formation Engine

Cel

"VIALACTEA will bring to a common forum the major new-generation surveys of the Galactic Plane from 1um to the radio, both in thermal continuum and in atomic and molecular lines, from Europe-funded space missions and ground-based facilities, to engage one of the fundamental challenges in Galactic astronomy: to quantify Galaxy-wide the relationship between the physical agents responsible for the onset and the regulation of star formation in a spiral galaxy and the resulting Rate and Efficiency of star formation, and obtain a ""star formation recipe"" that will be a cornerstone to trace the star formation history of galaxies back to their formation.
The new state-of-the-art Milky Way paradigm is offering today, for the first time, the possibility to deploy a coherent science analysis methodology that can be uniformly applied from the Galactic Center to the outskirts of the Galaxy. A homogeneous and inter-calibrated evolutionary classification of the cold and dense clumps hosting young forming clusters at a variety of evolutionary stages will allow to deliver a new 3D model of the Galaxy, mapping the essential critical parameters like column density thresholds, rate and efficiency of star formation in the Galaxy
To make such an analysis possible in a timely and effective fashion, we will develop a suite of next-generation 3D-visualization tools that will integrate visual analytics, on-the-fly handling of multi-SED radiative transfer modeling and data mining/machine-learning technologies to incorporate the astronomer's know-how into a set of supervised workflows with decision making capabilities.
The focus on research and analysis of data obtained from European space missions in combination with data from Europe-funded ground facilities, will enable time-effective exploitation of steradiant-scale multi-wavelength Galactic Plane surveys through new 3D-based visual analytics frameworks, making VIALACTEA's objectives timely and totally relevant for FP7-SPACE-2013-1."

Zaproszenie do składania wniosków

FP7-SPACE-2013-1
Zobacz inne projekty w ramach tego zaproszenia

Koordynator

ISTITUTO NAZIONALE DI ASTROFISICA
Adres
Viale Del Parco Mellini 84
00136 Roma
Włochy
Rodzaj działalności
Research Organisations
Wkład UE
€ 1 035 629,85
Kontakt administracyjny
Pietro Ubertini (Dr)

Uczestnicy (8)

UNIVERSITY OF LEEDS
United Kingdom
Wkład UE
€ 337 008
Adres
Woodhouse Lane
LS2 9JT Leeds
Rodzaj działalności
Higher or Secondary Education Establishments
Kontakt administracyjny
Martin Hamilton (Mr)
MAX-PLANCK-GESELLSCHAFT ZUR FORDERUNG DER WISSENSCHAFTEN EV
Niemcy
Wkład UE
€ 199 849,40
Adres
Hofgartenstrasse 8
80539 Munchen
Rodzaj działalności
Research Organisations
Kontakt administracyjny
Arnim Wolf
SZAMITASTECHNIKAI ES AUTOMATIZALASI KUTATOINTEZET
Węgry
Wkład UE
€ 120 750
Adres
Kende Utca 13-17
1111 Budapest
Rodzaj działalności
Research Organisations
Kontakt administracyjny
Reka Makkos (Ms)
CARDIFF UNIVERSITY
United Kingdom
Wkład UE
€ 212 230
Adres
Newport Road 30 36
CF24 0DE Cardiff
Rodzaj działalności
Higher or Secondary Education Establishments
Kontakt administracyjny
Rebecca Blackwell (Mrs)
UNIVERSITE D'AIX MARSEILLE
Francja
Wkład UE
€ 311 284
Adres
Boulevard Charles Livon 58 Le Pharo
13284 Marseille
Rodzaj działalności
Higher or Secondary Education Establishments
Kontakt administracyjny
Céline Damon (Ms)
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
Francja
Wkład UE
€ 190 879,60
Adres
Rue Michel Ange 3
75794 Paris
Rodzaj działalności
Research Organisations
Kontakt administracyjny
Gaelle Bujan (Mrs)
TOKAI NATIONAL HIGHER EDUCATION ANDRESEARCH SYSTEM, NATIONAL UNIVERSITY CORPORATION
Japonia
Wkład UE
€ 40 480
Adres
Furocho, Chikusa-ku, Aichi
464 8601 Nagoya
Rodzaj działalności
Higher or Secondary Education Establishments
Kontakt administracyjny
Yasuo Fukui (Prof)
THE UNIVERSITY OF EXETER
United Kingdom
Wkład UE
€ 40 480
Adres
The Queen's Drive Northcote House
EX4 4QJ Exeter
Rodzaj działalności
Higher or Secondary Education Establishments
Kontakt administracyjny
Gaynor Hughes (Ms)