GASP Publications
All GASP papers can be retrieved at the following public ADS library: ADS public libraryGASP. I. Gas stripping phenomena in galaxies with MUSE
Poggianti et al. (2017a), ApJ 844, 48, ArXiv #: 1704.05086GASP. II. A MUSE view of extreme ram-pressure stripping along the line of sight: kinematics of the jellyfish galaxy JO201
Bellhouse et al. (2017), ApJ 844, 49, ArXiv #: 1704.05087GASP. III. JO36: a case of multiple environmental effects at play?
Fritz et al. (2017), ApJ 848, 132, ArXiv #: 1704.05088GASP. IV. A Muse View of Extreme Ram-pressure Stripping in the Plane of the Sky: The Case of Jellyfish Galaxy JO204
Gullieuszik et al. (2017), ApJ 846, 27 ArXiv #: 1708.09035GASP. V. Ram-pressure stripping of a ring Hoag's-like galaxy in a massive cluster
Moretti et al. (2018a), MNRAS, 475, 4055 ArXiv #: 1802.07294Supermassive Black Holes Feed on Cosmic Jellyfish
Poggianti et al. (2017b), Nature, 548, 304 ArXiv #: 1708.09036GASP. VII. Signs of gas inflow onto a lopsided galaxy
Vulcani et al. (2018a), ApJ 852, 942 ArXiv #: 1802.07296GASP. VIII. Capturing the birth of a Tidal Dwarf Galaxy in a merging system at z~0.05
Vulcani et al. (2017c), ApJ 850, 163, ArXiv #: 1708.09037GASP IX. Jellyfish galaxies in phase-space: an orbital study of intense ram-pressure stripping in clusters
Jaffe et al. (2018), MNRAS 476, 4753, ArXiv #: 1802.07297GASP. X: APEX detection of molecular gas in the tails and in the disks of ram-pressure stripped galaxies
Moretti et al. (2018b), MNRAS 480, 2508, ArXiv #: 1803.06183Ultra-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
George et al. (2018), MNRAS 479, 4126, ArXiv #: 1803.06193GASP. XII. The variety of physical processes occurring in a single galaxy group in formation
Vulcani et al. (2018b), MNRAS, 480, 3152, ArXiv #: 1809.02668GASP. XIII. Star formation in gas outside galaxies
Poggianti et al. (2019a), MNRAS, 482, 4466, ArXiv #: 1811.00823Enhanced star formation in both disks and ram pressure stripped tails of GASP jellyfish galaxies
Vulcani et al. (2018c), ApJL, 866, 25 ArXiv #: 1810.05164GASP. XV. A MUSE View of Extreme Ram-Pressure Stripping along the Line of Sight: Physical properties of the Jellyfish Galaxy JO201
Bellhouse et al. (2019), MNRAS, 485, 1157, ArXiv #: 1902.04486GASP. XVI. Does cosmic web enhancement turn on star formation in galaxies?
Vulcani et al. (2019a), MNRAS, 487, 2278, ArXiv #: 1905.08971GASP. XVII. HI imaging of the jellyfish galaxy JO206: gas stripping and enhanced star formation
Ramatsoku et al. (2019), MNRAS,487, 4580, ArXiv #: 1906.03686GASP XVIII: Star formation quenching due to AGN feedback in the central region of a jellyfish galaxy
George et al. (2019), MNRAS, 487, 3102, ArXiv #: 1905.08973GASP - XIX. AGN and their outflows at the centre of jellyfish galaxies
Radovich et al. (2019), MNRAS, 486, 486, ArXiv #: 1905.08972GASP. XX. From the loose spatially-resolved to the tight global SFR-Mass relation in local spiral galaxies
Vulcani et al. (2019b), MNRAS 488, 1597, ArXiv #: 1907.00976GASP. XXI. Star formation rates in the tails of galaxies undergoing ram-pressure stripping
Gullieuszik et al. 2020, ApJ 899, 13, ArXiv #: 2006.16032GASP. XXII The molecular gas content of the JW100 jellyfish galaxy at z~0.05: does ram pressure promote molecular gas formation?
Moretti et al. (2020a), ApJ 889, 9, ArXiv #: 1912.06565GASP XXIII: A jellyfish galaxy as an astrophysical laboratory of the baryonic cycle
Poggianti et al. (2019b), ApJ 887,155, ArXiv #: 1910.11622GASP XXIV. The history of abruptly quenched galaxies in clusters
Vulcani et al. (2020a), ApJ 892, 146, ArXiv #: 2003.02274GASP XXV: Neutral Hydrogen gas in the striking Jellyfish Galaxy JO204
Deb et al. (2020), MNRAS 494, 5029, ArXiv #: 2004.04754GASP XXVI. HI Gas in Jellyfish Galaxies: The case of JO201 and JO206
Ramatsoku et al. (2020), A&A 640, 22, ArXiv #: 2006.11543GASP XXVII: Gas-phase metallicity scaling relations in disk galaxies with and without ram-pressure stripping
Franchetto et al. (2020), ApJ 895, 106, ArXiv #: 2004.11917Highly ordered magnetic fields in the tail of the jellyfish galaxy JO206
Mueller et al. (2021a), Nature Astronomy, 5, 159, ArXiv #: 2009.13287GASP XXIX. Unwinding the arms of spiral galaxies via ram-pressure stripping
Bellhouse et al. (2021), MNRAS, 500, 1285, ArXiv #: 2010.09733GASP XXX. The spatially resolved SFR-Mass relation in stripping galaxies in the local universe
Vulcani et al. (2020b), ApJ 899, 98, ArXiv #: 2007.04996The high molecular gas content, and the efficient conversion of neutral into molecular gas, in jellyfish galaxies
Moretti et al. (2020b), ApJL 897, 30, ArXiv #: 2006.13612GASP XXXII. Measuring the diffuse ionized gas fraction in ram-pressure stripped galaxies
Tomicic et al. (2021a), ApJ, 907, 22, ArXiv #: 2011.08869GASP XXXIII. The ability of spatially resolved data to distinguish among the different physical mechanisms affecting galaxies in low-density environments
Vulcani et al. (2021), ApJ 914, 27, ArXiv #: 2104.02089GASP XXXIV. Unfolding the thermal side of ram pressure stripping in the jellyfish galaxy JO201
Campitiello et al. (2021), ApJ, 911, 144, ArXiv #: 2013.03147GASP XXXV. Characteristics of the diffuse ionised gas in gas-stripped galaxies
Tomicic et al. (2021b), ApJ 922, 131, ArXiv #: 2108.12433GASP and MaNGA surveys shed light on the enigma of the gas metallicity gradients in disk galaxies
Franchetto et al. (2021a), ApJ 923, 28, ArXiv #: 2109.02656GASP XXXVII: The Most Extreme Jellyfish Galaxies Compared to Other Disk Galaxies in Clusters, an HI Study
Luber (2022), ApJ 927, 39, Arxiv #: 2111.02538GASP XXXVIII: The LOFAR-MeerKAT-VLA view on the non-thermal side of a jellyfish galaxy
Ignesti et al. (2022a), ApJ 924, 64, ArXiv #: 2201.00853GASP XXXIX: MeerKAT hunts Jellyfish in A2626
Deb et al. (2022), MNRAS 516, 2683, ArXiv #: 2208.12950Evidence for mixing between ICM and stripped ISM by the analysis of the gas metallicity in the tails of jellyfish galaxies
Franchetto at al. (2021b), ApJL 922, 6, ArXiv #: 2111.04755Exploring the AGN-ram pressure stripping connection in local clusters
Peluso et al. (2022), ApJ 927, 130, ArXiv #: 2111.02538The relevance of ram pressure stripping for the evolution of blue cluster galaxies as seen at optical wavelengths
Vulcani et al. (2022), ApJ 927, 91, ArXiv #: 2201.02644Walk on the Low Side: LOFAR explores the low-frequency radio emission of GASP jellyfish galaxies
Ignesti et al. (2022b), ApJ 937,58, ArXiv #: 2208.11955Unveiling the interplay between the GASP jellyfish galaxy JO194 and its environment with Chandra
Bartolini et al. (2022), ApJ 936,74, ArXiv #: 2208.01425GASP XLV: Stellar Bars In Jellyfish Galaxies. Analysis of ionised gas and stellar populations
Sanchez-Garcia et al. (2023), ApJ 945, 99, ArXiv #: 2301.06612Two striking head-tail galaxies in the galaxy cluster IIZW108: insights into transition to turbulence, magnetic fields, and particle re-acceleration
Mueller et al. (2021b), MNRAS 508, 5326, ArXiv #: 2110.03705A New Method to Constrain the Appearance and Disappearance of Observed Jellyfish Galaxy Tails
Smith et al. (2022), ApJ 934, 86, ArXiv #: 2207.00029Ultraviolet imaging observations of three jellyfish galaxies: star formation suppression in the centre and ongoing star formation in stripped tails
George et al. (2023), MNRAS 519, 2426, ArXiv #: 2212.02423The effect of cluster dynamical state on ram-pressure stripping
Lourenco et al. (2023), MNRAS 526 4831, ArXiv #: 2309.15934HST imaging of star-forming clumps in 6 GASP ram-pressure stripped galaxies
Giunchi et al. (2023a), ApJ 949, 72, ArXiv #: 2302.10615UV and H-alpha HST observations of 6 GASP jellyfish galaxies
Gullieuszik et al. (2023), ApJ 945, 54, ArXiv #: 2301.08279How Ram Pressure Drives Radial Gas Motions in the Surviving Disk
Akerman et al. (2023), ApJ 948, 18, ArXiv #: 2301.096523D modeling of the molecular gas kinematics in optically-selected jellyfish galaxies
Bacchini et al. (2023), ApJ 950, 24, ArXiv #: 2301.03090Radio continuum tails in ram pressure-stripped spiral galaxies: experimenting with a semi-empirical model in Abell 2255
Ignest et al. (2023a), A&A 675 118, ArXiv #: 2305.19941Ram pressure stripping in the EAGLE simulation
Kulier et al. (2023), ApJ 954 177, ArXiv #: 2305.03758Morphology of star-forming clumps in ram-pressure stripped galaxies as seen by HST
Giunchi et al. (2023b), ApJ 958, 73, ArXiv #: 2310.07267Spatially resolved comparison of SFRs from UV and H$\alpha$ in GASP gas-stripped galaxies
Tomicic et al. (2024), ApJ in press, ArXiv #: 2409.01351On the encounter between the GASP galaxy JO36 and the radio plume of GIN 049
Ignesti et al. (2023b), ApJ 956 122, ArXiv #: 2309.02002The morphological transformation of ram pressure stripped galaxies: a pathway from late to early galaxy types
Marasco et al. (2023), MNRAS 252 5359, ArXiv #: 2308.14791The evolution of the cold gas fraction in nearby clusters ram-pressure stripped galaxies
Moretti et al. (2023), ApJ 955 153, ArXiv #: 2309.00449Gas-phase metallicity of local AGN in the GASP and MaNGA surveys: the role of ram-pressure stripping
Peluso et al. (2023), ApJ 958 147, ArXiv #: 2309.05332The Surprising Lack of Effect from Stellar Feedback on the Gas Stripping Rate from Massive Jellyfish Galaxies
Akerman et al. (2024), MNRAS 527 9505, ArXiv #: 2311.04964The history of star-forming regions in the tails of 6 GASP jellyfish galaxies observed with the Hubble Space Telescope
Werle et al. (2024), A&A 682 162, ArXiv #: 2312.06879The radial orbits of ram-pressure-stripped galaxies in clusters from the GASP survey
Biviano et al. (2024), A&A 965 117, ArXiv #: 2403.02111Constraining the duration of ram pressure stripping features in the optical from the direction of jellyfish galaxy tails
Salinas et al. (2024), MNRAS 553 341, ArXiv #: 2408.03396Candidate ram-pressure stripped galaxies in six low-redshift clusters revealed from ultraviolet imaging
George et al. (2024), A&A in press, ArXiv #: 2409.10586The spatially resolved view of star formation in galaxy clusters
Poggianti et al. (2022), proceeding of IAUS373 in press 519, 2426, ArXiv #: 2211.12297Environmental processes at work in galaxy clusters: triggering of the AGN activity and development of X-ray tails
Moretti et al. (2022), Societa' Astronomica Italiana, 93, 108Integral field spectroscopy allows us to distinguish among the different physical mechanisms affecting galaxies in the different environments
Vulcani et al. (2023), Societa' Astronomica Italiana, 94, 2
High redshift science
Within the ERC program, some of us are conducting an effort to characterize ram pressure stripped galaxies in intermediate redshift clusters. Thanks to the MUSE-Guaranted Time Observations (GTO) data (Bacon et al. 2017, Richard et al 2021), 10 galaxy clusters at z=0.3-0.6 are being inspected and spatially resolved data of both star forming and passive cluster galaxies are being studied. Combining HST and MUSE observations we are characterizing the capability of ram pressure stripping in producing ionised gas tails and quenching the star formation at significant look-back times.
Observing ram pressure at work in intermediate redshift clusters with MUSE: the case of Abell 2744and Abell 370
Moretti et al. (2022), ApJ 925, 4, ArXiv #: 2111.04501Post-starburst galaxies in the centers of intermediate redshift clusters
Werle et al. (2022), ApJ 930, 43, ArXiv #: 2203.08862Locations and Morphologies of Jellyfish Galaxies in A2744 and A370
Bellhouse et al. (2022), ApJ 937, 18, ArXiv #: 2208.10524Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field
Vulcani et al. (2023), ApJL 948, 15 ArXiv #: 2303.01115Evidence for enhanced star formation rates in z~0.35 cluster galaxies undergoing ram pressure stripping
Vulcani et al. (2023), A&A in press ArXiv #: 2311.13486Gas Metallicity of Ram-Pressure Stripped Galaxies at Intermediate Redshift with MUSE Data
Khoram et al. (2024), A&A in press ArXiv #: 2042.13315
Complementary material associated with publications
Interactive online Figure for Bellhouse et al. (2017)
Here you can navigate the 3D visualisation of Hα gas of JO201, presented in Bellhouse et al. (2017). The gas has been extracted from the KUBEVIZ (Fossati et al. 2016) fit. X and Y axes show projected distance, with the Z axis representing the wavelength/velocity and linewidth/sigma. Surface contours are plotted with different colours, from yellow to dark blue. The units and contours are arbitrary as they have been chosen at levels which highlight interesting features in the Hα gas, such as the bright central emission, knots of Hα and the extended diffuse gas.
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Interact with mouse (drag to rotate, ctrl-drag to pan, scroll to zoom)