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Related papers: Star formation in HI tails: HCG 92, HCG 100 and 6 …

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Isolated compact groups of galaxies (CGs) present a range of dynamical states, group velocity dispersions, and galaxy morphologies with which to study galaxy evolution, particularly the properties of gas both within the galaxies and in the…

We present new Gemini/GMOS spectroscopic and archival imaging data of the interacting galaxy NGC 92, which is part of a compact group and displays an extended tidal tail. We have studied the physical properties of 20 star-forming complexes…

Compact groups are associations of a few galaxies in which the environment plays an important role in galaxy evolution. The low group velocity dispersion favors tidal interactions and mergers, which may bring stars from galaxies to the…

Astrophysics · Physics 2009-11-11 J. A. L. Aguerri , N. Castro-Rodriguez , N. Napolitano , M. Arnaboldi , O. Gerhard

We have used the GALEX ultraviolet telescope to study stellar populations and star formation morphology in a well-defined sample of 42 nearby optically-selected pre-merger interacting galaxy pairs. Galaxy interactions were likely far more…

Cosmology and Nongalactic Astrophysics · Physics 2010-01-08 Beverly J. Smith , Mark L. Giroux , Curtis Struck , Mark Hancock , Sabrina Hurlock

In a new HI imaging survey of Virgo galaxies (VIVA: VLA Imaging of Virgo galaxies in Atomic gas), we find 7 spiral galaxies with long HI tails. The morphology varies but all the tails are extended well beyond the optical radii on one side.…

Astrophysics · Physics 2010-11-04 Aeree Chung , J. H. van Gorkom , Jeffrey D. P. Kenney , Bernd Vollmer

We present a global study of HI spectral line mapping for 16 Hickson Compact Groups (HCGs) combining new and unpublished VLA data, plus the analysis of the HI content of individual galaxies. Sixty percent of the groups show morphological…

Astrophysics · Physics 2007-05-23 L. Verdes-Montenegro , M. S. Yun , B. A. Williams , W. K. Huchtmeier , A. Del Olmo , J. Perea

From R-band images of 42 Hickson compact groups, we present a sample of 47 candidate dwarf galaxies that are associated with the tidal tails and arms in the groups. The candidates, found in 15 tidal features, have R magnitudes and masses…

Astrophysics · Physics 2009-10-28 Sally D. Hunsberger , Jane C. Charlton , Dennis Zaritsky

I present observations of the Hickson Compact Group 88 (HCG88) obtained during the commissioning of a new 28-inch telescope at the Wise Observatory. This galaxy group was advertised to be non-interacting, or to be in a very early…

Astrophysics of Galaxies · Physics 2015-10-28 Noah Brosch

We investigate the properties of the B-band Tully-Fisher (T-F) relation for 25 compact group galaxies, using Vmax derived from 2-D velocity maps. Our main result is that the majority of the Hickson Compact Group galaxies lie on the T-F…

Astrophysics · Physics 2009-11-10 C. Mendes de Oliveira , P. Amram , H. Plana , C. Balkowski

Compact group galaxies often appear unaffected by their unusually dense environment. Closer examination can, however, reveal the subtle, cumulative effects of multiple galaxy interactions. Hickson Compact Group (HCG) 59 is an excellent…

Context. In spite of the numerous studies of low-luminosity galaxies in different environments, there is still no consensus about their formation scenario. In particular, a large number of galaxies displaying extremely low-surface…

Astrophysics of Galaxies · Physics 2016-11-30 A. V. Smith Castelli , F. R. Faifer , C. G. Escudero

We combine high resolution N-body simulations with deep observations of neutral hydrogen (HI) in nearby galaxy groups in order to explore two well-known theories of HI cloud formation: HI stripping by galaxy interactions and dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 Katie M. Chynoweth , Kelly Holley-Bockelmann , Emil Polisensky , Glen Langston

We have used V- and I- band images from the Hubble Space Telescope (HST) to identify compact stellar clusters within the tidal tails of twelve different interacting galaxies. The seventeen tails within our sample span a physical parameter…

We present results from a Spitzer, mid-infrared spectroscopy study of a sample of 74 galaxies located in 23 Hickson Compact Groups, chosen to be at a dynamically-active stage of HI depletion. We find evidence for enhanced warm H2 emission…

In this second paper of two analyses, we present near-infrared (NIR) morphological and asymmetry studies performed in sample of 92 galaxies found in different density environments: galaxies in Compact Groups (HCGs), Isolated Pairs of…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-19 I. Plauchu-Frayn , R. Coziol

We have obtained $H_{\alpha}$ fluxes and luminosities for a sample of 95 accordant galaxies from observations of 31 Hickson Compact Groups (HCGs) in the North hemisphere. This sample is the largest $H_{\alpha}$ selected catalogue of…

Astrophysics · Physics 2009-10-31 P. Severgnini , P. Saracco

We report the discovery of a very diverse set of five low-surface brightness (LSB) dwarf galaxy candidates in Hickson Compact Group 90 (HCG 90) detected in deep U- and I-band images obtained with VLT/VIMOS. These are the first LSB dwarf…

Extending deep observations of the neutral atomic hydrogen (HI) to the environment around galaxy groups can reveal a complex history of group interactions which is invisible to studies that focus on the stellar component. Hickson Compact…

About 20 percent of all nearby early-type galaxies ($M_{\star} \gtrsim 6 \times 10^{9}$ M$_{\odot}$) outside the Virgo cluster are surrounded by a disc or ring of low-column-density neutral hydrogen (HI) gas with typical radii of tens of…

Astrophysics of Galaxies · Physics 2016-10-26 Mustafa K. Yıldız , Paolo Serra , Reynier F. Peletier , Tom A. Oosterloo , Pierre-Alain Duc

Galaxies in Hickson Compact Group 91 (HCG 91) were observed with the WiFeS integral field spectrograph as part of our ongoing campaign targeting the ionized gas physics and kinematics inside star forming members of compact groups. Here, we…

Astrophysics of Galaxies · Physics 2015-05-20 F. P. A. Vogt , M. A. Dopita , S. Borthakur , L. Verdes-Montenegro , T. M. Heckman , M. S. Yun , K. C. Chambers