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Related papers: The peculiar galaxy IC 1182: An ongoing merger?

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We present IFU observations with MUSE@VLT and deep imaging with FORS@VLT of a dwarf galaxy recently formed within the giant collisional HI ring surrounding NGC 5291. This TDG-like object has the characteristics of typical z=1-2 gas-rich…

Astrophysics of Galaxies · Physics 2015-12-23 J. Fensch , P. -A. Duc , P. M. Weilbacher , M. Boquien , E. Zackrisson

We have found the peculiar galaxy NGC922 to be a new drop-through ring galaxy using multi-wavelength (UV-radio) imaging and spectroscopic observations. Its `C'-shaped morphology and tidal plume indicate a recent strong interaction with its…

We present an analysis of a 50ks XMM observation of the merging galaxy cluster ClJ0152.7-1357 at z=0.83. In addition to the two main subclusters and an infalling group detected in an earlier Chandra observation of the system, XMM detects…

Astrophysics · Physics 2009-11-13 B. J. Maughan , S. C. Ellis , L. R. Jones , K. O. Mason , F. A. Cordova , W. Priedhorsky

Using Hubble Space Telescope/Space Telescope Imaging Spectrograph G140M spectroscopy, we investigate an absorption-line system at $z$=0.07489 in the spectrum of the quasi-stellar object PG 1543+489 ($z_{QSO}$=0.401). The sightline passes…

Astrophysics of Galaxies · Physics 2019-02-27 Brenda Frye , David V. Bowen , Todd M. Tripp , Ed Jenkins , Max Pettini , Sara L. Ellison

We present a high-resolution (R~16,000) spectrum and a narrow-band image centered on the [NeII]12.8 micron line of the central kpc region of the starburst/Seyfert2 galaxy NGC 7582. The galaxy has a rotating circum-nuclear starburst disk,…

Astrophysics · Physics 2009-11-11 M. Wold , M. Lacy , H. U. Kaeufl , R. Siebenmorgen

The nearby S0 galaxy IC 5181 is studied to address the origin of the ionized gas component that orbits the galaxy on polar orbit. We perform detailed photometric and spectroscopic observations measuring the surface brightness distribution…

Astrophysics of Galaxies · Physics 2014-04-04 Alessandro Pizzella , Lorenzo Morelli , Enrico Maria Corsini , Elena Dalla Bonta` , Mary Cesetti

We present new important results about the intermediate-type Seyfert galaxy Mrk 315, recently observed through optical imaging and integral-field spectroscopy. Broad-band images were used to study the morphology of the host galaxy,…

Fossil groups are considered the end product in a galaxy group's evolution -- a massive central galaxy that dominates the luminosity budget of the group, as the outcome of efficient merging between intermediate-luminosity members. Little is…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 S. Lieder , S. Mieske , R. Sánchez-Janssen , M. Hilker , T. Lisker , M. Tanaka

We present interferometric observations of CO J=1-0 emission in the central regions of the edge-on galaxy NGC 4631, known for its extended gaseous halo and its tidal interactions. Previous single-dish observations revealed that almost all…

Astrophysics · Physics 2009-10-31 Richard J. Rand

Using Hubble Space Telescope (HST)/Cosmic Origins Spectrograph (COS) observations of one of the most metal-poor dwarf star-forming galaxies (SFG) in the local Universe, J2229+2725, we have discovered an extremely strong nebular CIV 1549,…

Astrophysics of Galaxies · Physics 2023-11-16 Y. I. Izotov , D. Schaerer , N. G. Guseva , T. X. Thuan , G. Worseck

We investigate the properties of a clump-cluster galaxy at redshift 1.57. The morphology of this galaxy is dominated by eight star-forming clumps in optical observations, and has photometric properties typical of most clump-cluster and…

The isolated elliptical (IE) NGC 7796 is accompanied by an interesting early-type dwarf galaxy, named NGC7796-DW1. It exhibits a tidal tail, very boxy isophotes, and multiple nuclei or regions (A, B, and C) that are bluer than the bulk…

Astrophysics of Galaxies · Physics 2018-12-19 T. Richtler , M. Hilker , K. Voggel , T. H. Puzia , R. Salinas , M. Gómez , R. Lane

The light of the merger remnant NGC 1316 is dominated by old and intermediate-age stars. The only sign of current star formation in this big galaxy is the HII region SH2, an isolated star cluster complex with a ring-like morphology and an…

Astrophysics of Galaxies · Physics 2017-05-24 T. Richtler , B. Husemann , M. Hilker , T. H. Puzia , F. Bresolin , M. Gómez

We present CO(1-0) and CO(2-1) maps of the Seyfert galaxy NGC 5728. Although a stellar nuclear bar structure is clearly identified in the near-infrared images in the central 10", inside the ring identified as the ILR of the primary bar,…

Astrophysics · Physics 2007-05-23 F. Combes , S. Leon

We present new high-resolution HI observations of the disk of the collisional infrared luminous (L$_{\rm IR}=2.2\times10^{11}$ L$_{\sun}$) galaxy NGC 1144, which reveal an apparent large-scale azimuthal and kinematic segregation of neutral…

Astrophysics · Physics 2008-11-26 P. N. Appleton , V. Charmandaris , Yu Gao , T. Jarrett , M. A. Bransford

We present new imaging at 12.81 and 11.7 microns of the central ~40"x30" (~0.7x0.5 kpc) of the starburst galaxy M82. The observations were carried out with the COMICS mid-infrared (mid-IR) imager on the 8.2m Subaru telescope, and are…

Astrophysics of Galaxies · Physics 2015-05-27 P. Gandhi , N. Isobe , M. Birkinshaw , D. M. Worrall , I. Sakon , K. Iwasawa , A. Bamba

Multi-line imaging of the nearby disk galaxy NGC 1482 with the Taurus Tunable Filter (TTF) on the Anglo-Australian Telescope reveals a remarkable hourglass-shaped [N II] 6583/H-alpha excitation structure suggestive of a galactic wind…

Astrophysics · Physics 2009-11-07 Sylvain Veilleux , David S. Rupke

Despite first being detected in the 1970s, surprisingly little is known about the OH main line maser population in the nearby starburst galaxy M82. Sometimes referred to as 'kilomasers', they have isotropic luminosities intermediate between…

The peculiar elliptical galaxy IC 1459 (M_V = -21.19, D = 16.5 Mpc) has a fast counterrotating stellar core, stellar shells and ripples, a blue nuclear point source and strong radio core emission. We present results of a detailed HST study…

Astrophysics · Physics 2009-10-31 G. A. Verdoes Kleijn , R. P. van der Marel , C. M. Carollo , P. T. de Zeeuw
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