Hα Morphologies and Environmental Effects in Virgo Cluster Spiral Galaxies

By R. Koopmann, J. Kenney. 2004

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In Astronomy and Astrophysics

Citations in the corpus

VLA IMAGING OF VIRGO SPIRALS IN ATOMIC GAS (VIVA). I. THE ATLAS AND THE H i PROPERTIES (2009, methodology): “In Figure 2, the optical and the UV images of the two galaxies that were not studied by Koopmann & Kenney (2004a, 2004b) are shown.”
THE GRISM LENS-AMPLIFIED SURVEY FROM SPACE (GLASS). I. SURVEY OVERVIEW AND FIRST DATA RELEASE (2015, background): “The power of spatially resolved information is exemplified by a study of Virgo which suggested that in the local universe stripping of gas is the main mechanism for quenching star formation rates in clusters (Koopmann & Kenney 2004).”
Environmental Effects on Late‐Type Galaxies in Nearby Clusters (2006, background): “Koopmann & Kenney (1998, 2004a, 2004b) and Koopmann et al. (2006), in their Ha imaging survey of 55 Virgo Cluster galaxies, found that a severe reduction of the star formation activity takes place only in the outer disks, producing truncated Ha profiles, with normal or possibly enhanced activity in…”
The ATLAS3D Project – XXX. Star formation histories and stellar population scaling relations of early-type galaxies (2015, unknown): “…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).”
BUDHIES II: a phase-space view of H i gas stripping and star formation quenching in cluster galaxies (2015, background): “(e.g. Dressler 1980; Lewis et al. 2002; Gómez et al. 2003; Koopmann & Kenney 2004; Boselli & Gavazzi 2006; Poggianti et al. 2006; Moran et al. 2007; Bamford et al. 2009; Jaffé et al. 2011b).”
The SAMI Galaxy Survey: Instrument specification and target selection (2014, background): “Furthermore, galaxy harassment (e.g. Moore, Lake & Katz 1998) or mergers and interactions between galaxies in groups and clusters can both strip gas and drive it towards the centre, triggering star formation (e.g. Iono, Yun & Mihos 2004; Koopmann & Kenney 2004).”
Galaxy Zoo: the dependence of morphology and colour on environment (2008, background): “…that star formation is enhanced in intermediat - density environments atz ∼ 0.6 (see also Bamford et al. 2005), in contrast to the independence (e.g., Balogh et al. 2004) orsuppression (e.g., Koopmann & Kenney 2004) of star formation with respect to increasing local density seen nowadays.”
LoCuSS: THE SLOW QUENCHING OF STAR FORMATION IN CLUSTER GALAXIES AND THE NEED FOR PRE-PROCESSING (2015, background): “…become strong enough to progressively strip their gas disks from the outside in (Brüggen & de Lucia 2008), producing truncated H I, H2 gas, and Hα disks (e.g., Koopmann & Kenney 2004; Boselli et al. 2006, 2014), and outer regions showing recently quenched stellar populations (Crowl & Kenney 2008).”
The SAURON project – VII. Integral-field absorption and emission-line kinematics of 24 spiral galaxy bulges (2006, background): “Koopmann & Kenney (2004), from Hα observations, reported a low level of star formation across the disc.”
The STAGES view of red spirals and dusty red galaxies: Mass-dependent quenching of star formation in cluster infall (2008, background): “The idea is that gas is gradually being stripped from galaxies, perhaps via ISM–ICM interaction, whereby the outer regions of a galaxy are swept first given their lower column densities (Koopmann & Kenney 2004b), and the truncation radius shrinks with time.”
GAS STRIPPING IN SIMULATED GALAXIES WITH A MULTIPHASE INTERSTELLAR MEDIUM (2009, methodology): “If we were to roughly classify these galaxies using the scheme of Koopmann & Kenney (2004), assuming that HII regions will follow our gas distribution, all three of our runs result in truncated disks.”