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Related papers: NGC 3310, a galaxy merger?

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NGC 3310 is a local galaxy with an intense, ongoing starburst thought to result from a merger with a companion galaxy. It has several known tidal features in the northwest and southern regions around the main galactic disc, as well as a…

NGC 4441 is a candidate for a merger between a spiral and an elliptical galaxy (S+E merger), because it shows typical tidal structures such as an optical tail and two shells. With a far-infrared luminosity of $\sim 5\cdot 10^9 L_{\odot}$…

Astrophysics · Physics 2009-11-13 Eva Manthey , Susanne Aalto , Susanne Huettemeister , Tom A. Oosterloo

Gas and star velocity dispersions have been derived for eight circumnuclear star-forming regions (CNSFRs) and the nucleus of the spiral galaxy NGC3310 using high resolution spectroscopy in the blue and far red. Stellar velocity dispersions…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Guillermo F. Hagele , Angeles I. Diaz , Monica V. Cardaci , Elena Terlevich , Roberto Terlevich

We present 1.4 GHz HI absorption line observations towards the starburst in NGC2146, made with the VLA and MERLIN. The HI gas has a rotating disk/ring structure with column densities between 6 and 18 x 10(21) atoms cm(-2). The HI absorption…

Astrophysics · Physics 2007-05-23 A. Tarchi , A. Greve , A. B. Peck , N. Neininger , K. A. Wills , A. Pedlar , U. Klein

Using deep 21-cm HI data from the Green Bank Telescope we have detected an ~18.3 kpc-long gaseous extension associated with the starbursting dwarf galaxy IC 10. The newly-found feature stretches 1.3 deg to the northwest and has a large…

We present MeerKAT observations of neutral hydrogen gas (HI) in the nearby merger remnant NGC 1316 (Fornax A), the brightest member of a galaxy group which is falling into the Fornax cluster. We find HI on a variety of scales, from the…

We describe the serendipitous discovery in the spectroscopic data of the Sloan Digital Sky Survey of a star-like object, SDSSJ103913.70+533029.7, at a heliocentric radial velocity of +1012 km/s. Its proximity in position and velocity to the…

Astrophysics · Physics 2008-11-26 G. R. Knapp , C. A. Tremonti , C. M. Rockosi

We present new radio continuum, 21 cm HI, and 2.6 mm CO data for the peculiar radio galaxy NGC 4410A and its companion NGC 4410B, and compare with available optical and X-ray maps. Our radio continuum maps show an asymmetric…

Astrophysics · Physics 2009-10-31 Beverly J. Smith

In this paper, we report the peculiar HI morphology of the cluster spiral galaxy NGC 6145, which has a 150 kpc HI filament on one side that is nearly parallel to its major axis. This filament is made up of several HI clouds and the diffuse…

Astrophysics of Galaxies · Physics 2017-08-02 Enci Wang , Jing Wang , Xu Kong , Fulai Guo , Lin Lin , Guobin Mou , Cheng Li , Ting Xiao

Broad and narrow band images and long slit spectroscopy of IC1182 are presented. The broad band images reveal a distorted morphology with a large, heavily obscured disk-like structure and several knots in the central region. Galactic…

Astrophysics · Physics 2016-08-16 M. Moles , D. Bettoni , G. Fasano , P. Kjærgaard , J. Varela

(abridged) Here we present HI line and 20-cm radio continuum data of the nearby galaxy pair NGC1512/1510 as obtained with the Australia Telescope Compact Array. These are complemented by GALEX UV-, SINGG Halpha- and Spitzer mid-infrared…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 Baerbel S. Koribalski , Angel R. Lopez-Sanchez

The Medusa (NGC 4194) is a well-studied nearby galaxy with the disturbed appearance of a merger and evidence for ongoing star formation. In order to test whether it could be the result of an interaction between a gas-rich disk-like galaxy…

Astrophysics · Physics 2009-11-13 E. Manthey , S. Huettemeister , S. Aalto , C. Horellou , P. Bjerkeli

The triggers of starburst episodes are a key component to our understanding of the baryon cycle in galaxies. Galaxy mergers are a commonly suggested catalyst for starbursts, but once the galaxies coalesce into a single kinematically…

An important open question is the relation between intracluster light and the halos of central galaxies in galaxy clusters. Here we report results from an on going project with the aim to characterize the dynamical state in the core of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 G. Ventimiglia , O. Gerhard , M. Arnaboldi , L. Coccato

We discuss new, high sensitivity HI observations of the spiral galaxy NGC2403 which show extended emission at anomalous velocities with respect to the `cold' disk. This `anomalous' gas component (~1/10 of the total HI mass) is probably…

Astrophysics · Physics 2009-11-07 Filippo Fraternali , Tom Oosterloo , Renzo Sancisi , Gustaaf van Moorsel

Early-type galaxies show a strong size evolution with redshift. This evolution is explained by fast "in-situ" star formation at high-$z$ followed by a late mass assembly mostly driven by minor mergers that deposit stars primarily in the…

We present new atomic hydrogen (HI) observations of the collisional ring galaxy NGC 922 obtained using the Australia Telescope Compact Array. Our observations reveal for the first time the vast extent of the HI disc of this galaxy. The HI…

Astrophysics of Galaxies · Physics 2018-04-20 Ahmed Elagali , O. Ivy Wong , Se-Heon Oh , Lister Staveley-Smith , Bärbel S. Koribalski , Kenji Bekki , Martin Zwaan

We present XMM-Newton EPIC observations of the two nearby starburst merger galaxies NGC 3256 & NGC 3310. The broad-band (0.3-10 keV) integrated X-ray emission from both galaxies shows evidence of multi-phase thermal plasmas plus an…

Astrophysics · Physics 2009-11-10 L. P. Jenkins , T. P. Roberts , M. J. Ward , A. Zezas

NGC 4013 is a nearby Sb edge-on galaxy known for its "prodigious" HI warp and its "giant" tidal stream. Previous work on this unusual object shows that it cannot be fitted satisfactorily by a canonical thin+thick disk structure. We have…

New deep VLA D array HI observations of the highly inclined nearby spiral galaxy NGC 2683 are presented. Archival C array data were processed and added to the new observations. To investigate the 3D structure of the atomic gas disk, we made…

Astrophysics of Galaxies · Physics 2016-02-17 B. Vollmer , F. Nehlig , R. Ibata
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