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Open AccessJournal ArticleDOI

Jellyfish Galaxy Candidates at Low Redshift

TLDR
In this article, the authors conducted a systematic search for galaxies that are being stripped of their gas at low-z (z=0.04-0.07) in different environments, selecting galaxies with varying degrees of morphological evidence for stripping.
Abstract
Galaxies that are being stripped of their gas can sometimes be recognized from their optical appearance. Extreme examples of stripped galaxies are the so-called ``jellyfish galaxies'', that exhibit tentacles of debris material with a characteristic jellyfish morphology. We have conducted the first systematic search for galaxies that are being stripped of their gas at low-z (z=0.04-0.07) in different environments, selecting galaxies with varying degrees of morphological evidence for stripping. We have visually inspected B and V-band images and identified 344 candidates in 71 galaxy clusters of the OMEGAWINGS+WINGS sample and 75 candidates in groups and lower mass structures in the PM2GC sample. We present the atlas of stripping candidates and a first analysis of their environment and their basic properties, such as morphologies, star formation rates and galaxy stellar masses. Candidates are found in all clusters and at all clustercentric radii, and their number does not correlate with the cluster velocity dispersion sigma or X-ray luminosity L_X. Interestingly, convincing cases of candidates are also found in groups and lower mass haloes (10^{11}-10^{14} M_{sun}), although the physical mechanism at work needs to be securely identified. All the candidates are disky, have stellar masses ranging from log M/M_{sun} 11.5 and the majority of them form stars at a rate that is on average a factor of 2 higher (2.5 sigma) compared to non-stripped galaxies of similar mass. The few post-starburst and passive candidates have weak stripping evidence. We conclude that the stripping phenomenon is ubiquitous in clusters and could be present even in groups and low mass haloes. Further studies will reveal the physics of the gas stripping and clarify the mechanisms at work.

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Citations
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Journal ArticleDOI

GASP. IX. Jellyfish galaxies in phase-space: an orbital study of intense ram-pressure stripping in clusters

TL;DR: In this article, the authors investigated the orbital histories of jellyfish galaxies in clusters and reconstruct their stripping history through position vs. velocity phase-space diagrams, and found that the jellyfish with the longest gas tails reside very near the cluster cores and are moving at very high speeds, which coincides with the conditions of the most intense ram-pressure.
Journal ArticleDOI

Ram-pressure feeding of supermassive black holes

TL;DR: Analysis of the galactic position and velocity relative to the cluster strongly supports the first hypothesis, and puts forward ram pressure as another possible mechanism for feeding the central supermassive black hole with gas.
References
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Journal ArticleDOI

On the variation of the initial mass function

TL;DR: In this paper, the uncertainty inherent in any observational estimate of the IMF is investigated by studying the scatter introduced by Poisson noise and the dynamical evolution of star clusters, and it is found that this apparent scatter reproduces quite well the observed scatter in power-law index determinations, thus defining the fundamental limit within which any true variation becomes undetectable.
Journal ArticleDOI

Galaxy harassment and the evolution of clusters of galaxies

TL;DR: In this article, the authors proposed that multiple high-speed encounters between galaxies (galaxy harassment) drive the morphological evolution in clusters, and showed that these encounters are very different from mergers; they transform small disk galaxies into dwarf elliptical or dwarf spheroidal galaxies.
Journal ArticleDOI

Galaxy bimodality due to cold flows and shock heating

TL;DR: In this paper, the authors address the origin of the robust bimodality observed in galaxy properties about a characteristic stellar mass ∼3 x 10 10 10 M ⊙, and propose that these features are driven by the thermal properties of the inflowing gas and their interplay with the clustering and feedback processes, all functions of the dark matter halo mass associated with a similar characteristic scale.
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