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GAs Stripping Phenomena in galaxies

Projektbeschreibung

Erkundung des gasförmigen Anteils der Galaxienbildung

Im Gehalt an kaltem Gas widerspiegelt sich in hohem Maße die Geschichte einer Galaxie sowie ihr Potenzial in Hinsicht auf die zukünftige Sternentstehung. Daher hat jeder physikalische Prozess, der den Gasgehalt einer Galaxie verändern könnte, wichtige Konsequenzen für ihre weitere Entwicklung. Hauptziel des EU-finanzierten Projekts GASP ist zu erforschen, wie, wann und warum in verschiedenen Umgebungen Gas aus Galaxien entfernt wird. Das Projekt wird auf riesige Datenmengen zurückgreifen, von denen die meisten mit dem MUSE-Instrument am Very Large Telescope der Europäischen Südsternwarte sowie mit ALMA, APEX und HST gesammelt wurden, um Prozesse dieser Art zu untersuchen. Die Projektergebnisse werden zum Wissen über Quallengalaxien beitragen, jene Galaxien, deren Gas scheinbar abhanden gekommen ist.

Ziel

The build up of galaxies is mainly driven by the availability of gas that can cool and form new stars. Any physical process that is able to alter the gas content of a galaxy has therefore important consequences for its evolution. The study of processes that can remove gas from galaxies is the subject of GASP (GAs Stripping Phenomena in galaxies), an ESO Large Program I am leading. GASP has obtained integral field spectroscopy (IFS) with MUSE of 114 low-z galaxies with masses in the range 10^9-10^11.5 Msun, hosted in X-ray selected clusters, in groups and filaments. The GASP sample includes the largest existing IFS sample of so- called “jellyfish galaxies” that have long tails of ionised gas, as well as other galaxies in different stages of ram pressure stripping in clusters and galaxies undergoing gas disturbance due to various phenomena in groups and filaments. GASP has the unique capability to combine the power of spatially resolved observations covering galaxy disks, outskirts and surroundings with the virtues of a statistical study of a significant number of galaxies. The MUSE GASP dataset, combined with ALMA, APEX, JVLA, UVIT and HST follow-up programs, form the basis for this ERC program. The goal is to accomplish an unprecedented break-through in our understanding of jellyfish galaxies, ram pressure stripping, gas removal processes in different environments and their consequences for the stellar history of galaxies. This multi faced, coherent program will investigate the physics of the baryonic cycle between the various gas phases (ionised, molecular and neutral) and the star formation under extreme conditions, the connection between ram pressure and AGN activity, the quenching of galaxies undergoing gas removal phenomena, and the physics of such phenomena in clusters, groups and filaments. The GASP ERC program will be a game changer in this field of research: there is no previous similar study, nor there can be a comparable one for quite a long time.

Finanzierungsplan

ERC-ADG - Advanced Grant

Gastgebende Einrichtung

ISTITUTO NAZIONALE DI ASTROFISICA
Netto-EU-Beitrag
€ 2 498 237,50
Adresse
VIALE DEL PARCO MELLINI 84
00136 Roma
Italien

Auf der Karte ansehen

Region
Centro (IT) Lazio Roma
Aktivitätstyp
Research Organisations
Links
Gesamtkosten
€ 2 498 237,50

Begünstigte (1)