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Opendata, web and dolomites

GASP SIGNED

GAs Stripping Phenomena in galaxies

Total Cost €

EC-Contrib. €

Partnership

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GASP project word cloud

Explore the words cloud of the GASP project. It provides you a very rough idea of what is the project "GASP" about.

stars galaxy basis virtues cycle quite cool ram molecular follow content 114 eso star disks remove alma game mainly ionised faced erc hosted undergoing agn unprecedented combine quenching time spectroscopy 9 extreme break integral subject history environments power physical baryonic groups form filaments uvit evolution jvla nor observations neutral disturbance 10 programs gasp statistical phases apex capability tails outskirts hst gas dataset galaxies removal stripping combined pressure physics muse 11 jellyfish am msun phenomena coherent alter connection resolved changer masses stages ray clusters surroundings ifs stellar

Project "GASP" data sheet

The following table provides information about the project.

Coordinator	ISTITUTO NAZIONALE DI ASTROFISICA Organization address address: VIALE DEL PARCO MELLINI 84 city: ROMA postcode: 136 website: www.inaf.it contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.
Coordinator Country	Italy [IT]
Total cost	2˙498˙237 €
EC max contribution	2˙498˙237 € (100%)
Programme	1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
Code Call	ERC-2018-ADG
Funding Scheme	ERC-ADG
Starting year	2019
Duration (year-month-day)	from 2019-06-01 to 2024-05-31

Partnership

Take a look of project's partnership.

#	participants	country	role	EC contrib. [€]
1	ISTITUTO NAZIONALE DI ASTROFISICA ISTITUTO NAZIONALE DI ASTROFISICA Organization address address: VIALE DEL PARCO MELLINI 84 city: ROMA postcode: 136 website: www.inaf.it contact info title: n.a. name: n.a. surname: n.a. function: n.a. email: n.a. telephone: n.a. fax: n.a.	IT (ROMA)	coordinator	2˙498˙237.00

Map

Project objective

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.

Publications

List of publications.
year	authors and title	journal	last update
2019	Benedetta Vulcani, Bianca M Poggianti, Alessia Moretti, Andrea Franchetto, Marco Gullieuszik, Jacopo Fritz, Daniela Bettoni, Stephanie Tonnesen, Mario Radovich, Yara L JaffÃ©, Sean McGee, Callum Bellhouse, Giovanni Fasano GASP â€“ XX. From the loose spatially resolved to the tight global SFRâ€“mass relation in local spiral galaxies published pages: 1597-1617, ISSN: 0035-8711, DOI: 10.1093/mnras/stz1829	Monthly Notices of the Royal Astronomical Society 488/2	2019-08-29

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The information about "GASP" are provided by the European Opendata Portal: CORDIS opendata.