Jellyfish galaxy candidates in MACS J0717.5+3745 and thirty-nine other clusters of the DAFT/FADA and CLASH surveys
arXiv:2102.02595 · doi:10.1051/0004-6361/202039770
Abstract
Galaxies in clusters undergo several phenomena such as ram pressure stripping and tidal interactions, that can trigger or quench their star formation and, in some cases, lead to galaxies acquiring unusual shapes and long tails. We searched for jellyfish galaxy candidates in a sample of 40 clusters from the DAFT/FADA and CLASH surveys covering the redshift range 0.2<z<0.9. In MACS J0717.5+3745 (MACS0717), our large spatial coverage and abundant sampling of spectroscopic redshifts allowed us to pursue a detailed analysis of jellyfish galaxy candidates in this cluster and its extended filament. We looked at the Hubble Space Telescope images of all the cluster galaxies (based on redshifts), and classified them as a function of their likeliness to be jellyfish galaxies, and give catalogues of jellyfish candidates with positions, redshifts, magnitudes, and projected distance to the respective cluster centre. We found 81 jellyfish candidates in the extended region around MACS0717, and 97 in 22 other clusters. Jellyfish galaxy candidates in MACS0717 tend to avoid the densest regions of the cluster, while this does not appear to be the case in the other clusters. For 79 galaxies in MACS0717 and 31 in other clusters, we computed the best stellar population fits with LePhare through the GAZPAR interface. We find that jellyfish candidates tend to be star forming objects, with blue colours, young ages, high star formation rates and specific star formation rates. In a SFR versus stellar mass diagram, jellyfish galaxy candidates appear to have somewhat larger SFRs than non-jellyfish star forming galaxies Based on several arguments, the jellyfish candidates identified in MACS0717 seem to have fallen rather recently into the cluster. A very rough estimate of the proportions of jellyfish galaxies in the studied clusters is about 10%.
Accepted for publication in Astronomy & Astrophysics
References in corpus (24)
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- Detection of quiescent galaxies in a bicolor sequence from z=0-2
- The relation between velocity dispersion and mass in simulated clusters of galaxies: dependence on the tracer and the baryonic physics
- MUSE sneaks a peek at extreme ram-pressure stripping events. I. A kinematic study of the archetypal galaxy ESO137-001
- The strong transformation of spiral galaxies infalling into massive clusters at z~0.2
- Ram pressure feeding super-massive black holes
- Abundant molecular gas and inefficient star formation in intracluster regions: Ram pressure stripped tail of the Norma galaxy ESO137-001
- Strange filamentary structures ("fireballs") around a merger galaxy in the Coma cluster of galaxies
- GASP XXIII: A jellyfish galaxy as an astrophysical laboratory of the baryonic cycle
- GASP. XXII The molecular gas content of the JW100 jellyfish galaxy at z~0.05: does ram pressure promote molecular gas formation?
- GASP XXI. Star formation rates in the tails of galaxies undergoing ram-pressure stripping
- The spatial distribution of galaxies of different spectral types in the massive intermediate-redshift cluster MACSJ0717.5+3745
- An X-ray/optical study of the complex dynamics of the core of the massive intermediate-redshift cluster MACSJ0717.5+3745
- GASP XXIX -- Unwinding the arms of spiral galaxies via ram-pressure stripping
- 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?
- Star formation in the massive cluster merger Abell 2744
- GASP XIX: AGN and their outflows at the center of jellyfish galaxies
- Ten Billion Years of Brightest Cluster Galaxy Alignments
- Galaxy cluster mergers as triggers for the formation of jellyfish galaxies: case study of the A901/2 system
- Physical properties of Brightest Cluster Galaxies up to redshift 1.80 based on HST data
- The link between brightest cluster galaxy properties and large scale extensions of 38 DAFT/FADA and CLASH clusters in the redshift range 0.2<z<0.9
- Jellyfish: Resolving the kinematics of extreme ram-pressure stripping at
- Explaining the enhanced star formation rate of Jellyfish galaxies in galaxy clusters
Cited by in corpus (21)
- Ram Pressure Stripping in High-Density Environments
- The relevance of ram pressure stripping for the evolution of blue cluster galaxies as seen at optical wavelengths
- Observing ram pressure at work in intermediate redshift clusters with MUSE: the case of Abell 2744and Abell 370
- LoTSS Jellyfish Galaxies IV: Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949
- A New Method to Constrain the Appearance and Disappearance of Observed Jellyfish Galaxy Tails
- Quantifying the role of ram pressure stripping of galaxies within galaxy groups
- The MUSE view of ram pressure stripped galaxies in clusters: the GASP sample
- Enhanced Star Formation Activity of Extreme Jellyfish Galaxies in Massive Clusters and the Role of Ram Pressure Stripping
- Investigating the delay between dust radiation and star-formation in local and distant quenching galaxies
- The effect of cluster dynamical state on ram-pressure stripping
- Locations and Morphologies of Jellyfish Galaxies in A2744 and A370
- A GMOS/IFU Study of Jellyfish Galaxies in Massive Clusters
- Spatially resolved self-consistent spectral modelling of jellyfish galaxies from MUSE with FADO: trends with mass and stripping intensity
- Star formation across cosmic time
- Comparing the interstellar and circumgalactic origin of gas in the tails of jellyfish galaxies
- Ram pressure stripping in the z~0.5 galaxy cluster MS 0451.6-0305
- Euclid: Early Release Observations of ram-pressure stripping in the Perseus cluster. Detection of parsec scale star formation with in the low surface brightness stripped tails of UGC 2665 and MCG +07-07-070
- Identification of ram pressure stripping features in galaxies using citizen science
- Identifying Astrophysical Anomalies in 99.6 Million Cutouts from the Hubble Legacy Archive Using AnomalyMatch
- With arms wide open: a VLT/MUSE view of the mechanisms driving unwinding spiral arms in cluster galaxies
- What goes around comes around: the fate of stars in stripped tails of gas