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Related papers: Virgo Early-Type Dwarfs in ALFALFA

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Because of its proximity and richness on late-type galaxies, the Virgo cluster has been the subject of numerous studies exploring the effect of the intracluster environment on galaxy evolution. First discovered nearly three decades ago by…

Astrophysics · Physics 2007-05-23 J. M. Solanes

We present the results of a search for clusters in dwarf irregular galaxies in the Virgo and Fornax Cluster using HST WFPC2 snapshot data. The galaxy sample includes 28 galaxies, 11 of which are confirmed members of the Virgo and Fornax…

Astrophysics · Physics 2009-11-10 Anil Seth , Knut Olsen , Bryan Miller , Jennifer Lotz , Rosie Telford

We present a study of ultra compact dwarf (UCD) galaxies in the Virgo cluster based mainly on imaging from the Next Generation Virgo Cluster Survey (NGVS). Using $\sim$100 deg$^{2}$ of $u^*giz$ imaging, we have identified more than 600…

We present stellar age profiles for 64 Virgo cluster disk galaxies whose analysis poses a challenge for current galaxy formation models. Our results can be summarized as follows: first, and contrary to observations of field galaxies, these…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Joel C. Roediger , Stephane Courteau , Patricia Sanchez-Blazquez , Michael McDonald

We present integral-field spectroscopy of 27 galaxies in the Coma cluster observed with the Oxford SWIFT spectrograph, exploring the kinematic morphology-density relationship in a cluster environment richer and denser than any in the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 R. C. W. Houghton , Roger L. Davies , F. D'Eugenio , N. Scott , N. Thatte , F. Clarke , M. Tecza , G. S. Salter , L. M. R. Fogarty , T. Goodsall

We present a systematic search for disks in 476 Virgo cluster early-type dwarf (dE) galaxies. Disk features (spiral arms, edge-on disks, or bars) were identified by applying unsharp masks to a combined image from three bands (g, r, i), as…

Astrophysics · Physics 2009-11-11 Thorsten Lisker , Eva K. Grebel , Bruno Binggeli

The impact of the cluster environment on the evolution of dwarf galaxies is investigated by comparing the properties of a sample of dwarf irregulars (dIs) in the Virgo Cluster with a control sample of nearby ("field") dIs having oxygen…

Astrophysics · Physics 2009-11-07 Henry Lee , Marshall L. McCall , Michael G. Richer

Keck/ESI spectroscopy is presented for six Virgo Cluster dwarf elliptical (dE) galaxies. The mean line-of-sight velocity and velocity dispersion are resolved as a function of radius along the major axis of each galaxy, nearly doubling the…

Astrophysics · Physics 2009-11-07 M. Geha , P. Guhathakurta , R. van der Marel

We present 21 cm observations of a 5 x degree region in the Virgo cluster, obtained as part of the Arecibo Galaxy Environment Survey. 13 cluster members are detected, together with 36 objects in the background. We compare and contrast the…

Astrophysics of Galaxies · Physics 2015-06-11 R. Taylor , J. I. Davies , R. Auld , R. F. Minchin , R. Smith

We present the results of a Keck-ESI study of dwarf galaxies across a range of environment: the Perseus Cluster, the Virgo Cluster, the NGC 1407 group, and the NGC 1023 group. Eighteen dEs are targeted for spectroscopy, three for the first…

Astrophysics of Galaxies · Physics 2015-09-23 Samantha J. Penny , Joachim Janz , Duncan A. Forbes , Andrew J. Benson , Jeremy Mould

(Abridged) The distances and HI contents of 161 spiral galaxies in the region of Virgo cluster are used to gain insight into the complicated structure of this galaxy system. The 3D galaxy distribution has been inferred from quality distance…

Astrophysics · Physics 2009-11-07 J. M. Solanes , T. Sanchis , E. Salvador-Sole , R. Giovanelli , M. P. Haynes

We study star-formation-inducing mechanisms in galaxies through multi- wavelength measurements of a sample of dwarf galaxies in the Virgo cluster described in paper I. Our main goal is to test how star formation inducing mechanisms depend…

Astrophysics · Physics 2008-02-03 Elchanan Almoznino , Noah Brosch

Although cluster dwarf galaxies are often neglected due to their faintness, recent observations demonstrate that they are critical for understanding the physical processes behind galaxy and cluster formation. Dwarfs are the most common…

Astrophysics · Physics 2007-05-23 Christopher J. Conselice

The study of dwarf galaxies in groups is a powerful tool for investigating galaxy evolution, chemical enrichment and environmental effects on these objects. Here we present results obtained for dwarf galaxies in the Centaurus A complex, a…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 D. Crnojević , E. K. Grebel , A. A. Cole , A. Koch , M. Rejkuba , G. Da Costa , H. Jerjen

The results of an Halpha photometric survey of 30 dwarf galaxies of various morphologies in the Centaurus A and Sculptor groups are presented. Of these 30, emission was detected in 13: eight are of late-type, two are early-type and three…

Astrophysics · Physics 2009-11-13 A. Bouchard , G. S. Da Costa , H. Jerjen

Quantitative measures of central light concentration and star formation activity are derived from R and Halpha surface photometry of 84 bright S0-Scd Virgo Cluster and isolated spiral galaxies. For isolated spirals, there is a good…

Astrophysics · Physics 2009-10-30 R. A. Koopmann , J. D. P. Kenney

We present the Halpha imaging observations of 273 late-type galaxies in the nearby rich galaxy clusters Virgo, A1367, Coma, Cancer, Hercules and in the Great Wall, carried out primarily with the 2.1m telescope of the San Pedro Martir…

Astrophysics · Physics 2009-11-11 G. Gavazzi , A. Boselli , L. Cortese , I. Arosio , A. Gallazzi , P. Pedotti , L. Carrasco

We present the color distributions of globular cluster (GC) systems for 100 Virgo cluster early-type galaxies observed in the ACS Virgo Cluster Survey. The color distributions of individual GC systems are consistent with continuous trends…

Halpha+[NII] imaging observations of 369 late-type galaxies in the Virgo cluster and in the Coma/A1367 supercluster are analyzed. They constitute an optically selected sample (m_p<16.0) observed with 60% c.a. completeness.These observations…

Astrophysics · Physics 2009-11-07 G. Gavazzi , A. Boselli , P. Pedotti , A. Gallazzi , L. Carrasco
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