The role of environment on quenching, star formation and AGN activity
arXiv:2005.03735 · doi:10.1017/S1743921320002070
Abstract
Galaxies undergoing ram pressure stripping in clusters are an excellent opportunity to study the effects of environment on both the AGN and the star formation activity. We report here on the most recent results from the GASP survey. We discuss the AGN-ram pressure stripping connection and some evidence for AGN feedback in stripped galaxies. We then focus on the star formation activity, both in the disks and the tails of these galaxies, and conclude drawing a picture of the relation between multi-phase gas and star formation.
arXiv commentProceedings of the IAU Symposium 359 "Galaxy evolution and feedback across different environments", editors T. Storchi-Bergmann, R. Overzier, W. Forman & R. Riffel - final version
References in corpus (46)
- GASP I: Gas stripping phenomena in galaxies with MUSE
- VLA HI Observations of Gas Stripping in the Virgo Cluster Spiral NGC 4522
- Gas Stripping in Simulated Galaxies with a Multiphase ISM
- Jellyfish: Evidence of extreme ram-pressure stripping in massive galaxy clusters
- MUSE sneaks a peek at extreme ram-pressure stripping events. I. A kinematic study of the archetypal galaxy ESO137-001
- Ultraviolet tails and trails in cluster galaxies: A sample of candidate gaseous stripping events in Coma
- A dozen new galaxies caught in the act: Gas stripping and extended emission line regions in the Coma cluster
- GASP IX. Jellyfish galaxies in phase-space: an orbital study of intense ram-pressure stripping in clusters
- Enhanced star formation in both disks and ram pressure stripped tails of GASP jellyfish galaxies
- Spectacular X-ray tails, intracluster star formation and ULXs in A3627
- Ram pressure feeding super-massive black holes
- MUSE sneaks a peek at extreme ram-pressure stripping events. II. The physical properties of the gas tail of ESO137-001
- Abundant molecular gas and inefficient star formation in intracluster regions: Ram pressure stripped tail of the Norma galaxy ESO137-001
- GASP XIII. Star formation in gas outside galaxies
- Star Formation in Ram Pressure Stripped Tails
- Caught in the Act: Strong, Active Ram Pressure Stripping in Virgo Cluster Spiral NGC 4330
- ACCESS - V. Dissecting ram-pressure stripping through integral-field spectroscopy and multi-band imaging
- ALMA unveils widespread molecular gas clumps in the ram pressure stripped tail of the Norma jellyfish galaxy
- Molecular Gas Dominated 50 kpc Ram Pressure Stripped Tail of the Coma Galaxy D100
- GASP II. A MUSE view of extreme ram-pressure stripping along the line of sight: kinematics of the jellyfish galaxy JO201
- IC 3418: Star Formation in a Turbulent Wake
- GASP IV: A muse view of extreme ram-pressure stripping in the plane of the sky: the case of jellyfish galaxy JO204
- GASP III. JO36: a case of multiple environmental effects at play?
- GASP XXIII: A jellyfish galaxy as an astrophysical laboratory of the baryonic cycle
- GASP. X: APEX detection of molecular gas in the tails and in the disks of ram-pressure stripped galaxies
- The SAMI Galaxy Survey: Quenching of star formation in clusters I. Transition galaxies
- GASP. XXII The molecular gas content of the JW100 jellyfish galaxy at z~0.05: does ram pressure promote molecular gas formation?
- Star formation in shocked cluster spirals and their tails
- Ram pressure stripping of disc galaxies orbiting in clusters. II. Galactic wakes
- Spectacular HST observations of the Coma galaxy D100 and star formation in its ram pressure stripped tail
- GASP XVII. HI imaging of the jellyfish galaxy JO206: gas stripping and enhanced star formation
- Ultra-Violet Imaging Telescope view of ram-pressure stripping in action: Star formation in the stripped gas of the GASP jellyfish galaxy JO201 in Abell 85
- MHD simulations of ram pressure stripping of a disk galaxy
- GASP. XV. A MUSE View of Extreme Ram-Pressure Stripping along the Line of Sight: Physical properties of the Jellyfish Galaxy JO201
- GASP. XVI. Does cosmic web enhancement turn on star formation in galaxies?
- GASP XXIV. The history of abruptly quenched galaxies in clusters
- GASP. XII. The variety of physical processes occurring in a single galaxy group in formation
- GASP XIX: AGN and their outflows at the center of jellyfish galaxies
- GASP XVIII: Star formation quenching due to AGN feedback in the central region of a jellyfish galaxy
- OMEGA -- OSIRIS Mapping of Emission-line Galaxies in A901/2 -- V. The rich population of jellyfish galaxies in the multi-cluster system Abell 901/2
- GASP. XX. From the loose spatially-resolved to the tight global SFR-Mass relation in local spiral galaxies
- The ALMA Detection of Extraplanar 13CO in a Ram-pressure-stripped Galaxy and Its Implication
- GASP XXV: Neutral Hydrogen gas in the striking Jellyfish Galaxy JO204
- GASP. V. Ram-pressure stripping of a ring Hoag's-like galaxy in a massive cluster
- GASP. VII. Gas accretion onto an isolated galaxy
- GASP VIII: Capturing the birth of a Tidal Dwarf Galaxy in a merging system at z~0.05