VLA IMAGING OF VIRGO SPIRALS IN ATOMIC GAS (VIVA). I. THE ATLAS AND THE H i PROPERTIES

By A. Chung, J. V. van Gorkom, J. Kenney, H. Crowl, B. Vollmer. 2009

427 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

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Citations in the corpus

• MUSE sneaks a peek at extreme ram-pressure stripping events - I. A kinematic study of the archetypal galaxy ESO137-001 (2014, background): “More c© xxxx RAS significantly, these gas-deficient galaxies, and particularly those residing near the cluster cores, often exhibit truncated and disturbed gas disks (e.g. Vollmer et al. 2008; Chung et al. 2009) or, in some cases, one-sidedH I tails (e.g. Chung et al. 2007).”
• The ATLAS3D project - XIII. Mass and morphology of H I in early-type galaxies as a function of environment (2011, methodology): “The above results are in good agreement with conclusions from the VIVA H I survey of spirals in Virgo by Chung et al. (2009).”
• Galaxy evolution in groups and clusters: satellite star formation histories and quenching time-scales in a hierarchical Universe (2012, background): “More drastically, in the extreme case of both high gas density and satellite velocity, ram-pressure can strip cold gas directly from the disc (Gunn & Gott 1972; Abadi et al. 1999; Chung et al. 2009).”
• A UNIVERSAL, LOCAL STAR FORMATION LAW IN GALACTIC CLOUDS, NEARBY GALAXIES, HIGH-REDSHIFT DISKS, AND STARBURSTS (2011, neutral): “In nearby disk galaxies σ ≈ 8 km s−1, with less than a factor of 2 variation either within a single galaxy or between different galaxies (Dib et al. 2006; Walter et al. 2008; Chung et al. 2009), which means that tff is nearly independent of galactic properties in this regime.”
• Ultraviolet tails and trails in cluster galaxies: a sample of candidate gaseous stripping events in Coma (2010, result): “The HI tails are all pointing away from the centre of Virgo.”
• The ATLAS3D Project – XXX. Star formation histories and stellar population scaling relations of early-type galaxies (2015, result): “…is qualitatively consistent with an extension of what is found in Virgo late-type galaxies, where the intracluster medium appears to truncate extended neutral gas discs with subsequent implications on star formation activity (Koopmann & Kenney 2004; Crowl & Kenney 2008; Chung et al. 2009).”
• The ATLAS3D project – IV. The molecular gas content of early-type galaxies (2011, result): “This behaviour is markedly different from that of the atomic gas in the spirals of the Virgo cluster, which show strong H I deficiencies near the centre of the cluster (Cayatte et al. 1990; Chung et al. 2009).”
• Galaxy evolution in groups and clusters: star formation rates, red sequence fractions and the persistent bimodality (2011, background): “There are striking, direct examples of rampressure stripping occurring for satellites in nearby clusters (e.g. Chung et al. 2009), some of which are even near the virial radius.”
• THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE SURVEY (2012, methodology): “…0.6 mJy beam−1 will soon be available from the Arecibo Galaxy Environment Survey (AGES; J. E. Taylor et al. 2012, in preparation), while higher resolution 15′′ VLA H i data for 53 late-type galaxies is available from the VLA Imaging of Virgo Spirals in Atomic Gas survey (VIVA; Chung et al. 2009a).”
• A REVISED PARALLEL-SEQUENCE MORPHOLOGICAL CLASSIFICATION OF GALAXIES: STRUCTURE AND FORMATION OF S0 AND SPHEROIDAL GALAXIES (2011, background): “Many spiral galaxies near the center of the cluster show H I tails; the above authors interpret them as gas that is being stripped by the hot, X-ray-emitting gas that pervades the cluster (see Chung et al. 2009 for an update and van Gorkom & Kenney 2011 for a review).”
• BUDHIES II: a phase-space view of H i gas stripping and star formation quenching in cluster galaxies (2015, background): “Their morphologies and stellar populations, together with an observational estimate of their orbital histories, suggest these galaxies have been stripped in the outskirts of clusters, before crossing the centre (Chung et al. 2009; Crowl & Kenney 2008; Kenney et al. 2004).”
• Cold gas stripping in satellite galaxies: from pairs to clusters (2016, methodology): “…cold gas (∼102 K) show that reservoirs are adversely affected in the highest density environments such as galaxy clusters (Giovanelli & Haynes 1985; Chung et al. 2009; Cortese et al. 2011; Serra et al. 2012), and that gas processing begins to occur within the group environment (Kilborn et al.…”
• SPARC: MASS MODELS FOR 175 DISK GALAXIES WITH SPITZER PHOTOMETRY AND ACCURATE ROTATION CURVES (2016, background): “Galaxies in dense clusters like Virgo may show smaller values of RH I/R? due to gas stripping (e.g., Chung et al. 2009).”
• The GALEX Arecibo SDSS Survey - VIII. Final data release. The effect of group environment on the gas content of massive galaxies (2013, background): “…show that Hi is removed from the star-forming disk (Gavazzi 1989; Cayatte et al. 1990; Bravo-Alfaro et al. 2000; Kenney, van Gorkom & Vollmer 2004; Chung et al. 2009), mainly due to ram pressure stripping by the dense intracluster medium through which galaxies move (Gunn & Gott 1972; Vollmer…”
• The ATLAS3D project - VII. A new look at the morphology of nearby galaxies: the kinematic morphology-density relation (2011, result): “The importance of the IGM near the cluster core (R < 0.5 Mpc) is also evident in the studies of Chung et al. (2007, 2009), who find only truncated and displaced H I disks in spirals in that region, while more extended and regular disks reside further out.”
• GASP. I. Gas Stripping Phenomena in Galaxies with MUSE (2017, background): “…of ram-pressure stripping of the neutral gas in nearby galaxy clusters (e.g., Haynes et al. 1984; Cayatte et al. 1990; Kenney et al. 2004; Chung et al. 2009; Vollmer et al. 2010; Jaffé et al. 2015)and sometimes also in groups (e.g., Verdes-Montenegro et al. 2001; Rasmussen et al. 2006;…”