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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.

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

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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