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GASP: Gas stripping and the outskirts of galaxies as a function of environment

Published online by Cambridge University Press:  21 March 2017

Bianca Poggianti  and
the GASP team
Bianca Poggianti
Affiliation:
INAF-Astronomical Observatory of Padova vicolo dell’Osservatorio 5, 35122, Padova, Italy email: bianca.poggianti@oapd.inaf.it
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Abstract

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We present GASP, an ongoing ESO Large Program with MUSE aiming to study gas removal processes from galaxies at low redshift. GASP targets 100 galaxies with tails, tentacles and one-sided debris. MUSE data allows a detailed investigation of the ionized stripped gas, as well as of the gas and stars within the galaxy out to large distances from the galaxy center. We show the first results for two of the GASP galaxies that are striking cluster jellyfish galaxies of stellar masses ~ 1011M⊙.

Keywords

Galaxies:evolutiongalaxy:intergalactic mediumgalaxies:ISMgalaxies:peculiar
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S321: Formation and Evolution of Galaxy Outskirts , March 2016 , pp. 202 - 204
Copyright
Copyright © International Astronomical Union 2017 

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