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Related papers: Vertically Extended Neutral Gas in the Massive Edg…

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We discuss the distribution and kinematics of neutral hydrogen in the halos of spiral galaxies. We focus in particular on new results obtained for the nearby Sc galaxy NGC 2403 which have revealed the presence of extended HI emission (here…

Astrophysics · Physics 2007-05-23 Renzo Sancisi , Filippo Fraternali , Tom Oosterloo , Gustaaf van Moorsel

A significant fraction of baryons in galaxies are in the form of diffuse gas of the circumgalactic medium (CGM). One critical component of the multi-phases of CGM, the so-called "coronal" warm-hot phase gas ($\rm 10^{5}-10^{6}$ K) traced by…

Astrophysics of Galaxies · Physics 2021-07-21 Haeun Chung , Carlos J. Vargas , Erika Hamden

NGC 2146, a nearby luminous infrared galaxy (LIRG), presents evidence for outflows along the disk minor axis in all gas phases (ionized, neutral atomic and molecular). We present an analysis of the multi-phase starburst driven superwind in…

We present results from a study of the NGC 4756 group which is dominated by the elliptical galaxy NGC 5746. The characteristics of the group are investigated through (a) the detailed investigation of the morphological, photometric and…

Astrophysics · Physics 2009-11-10 R. Gruetzbauch , B. Kelm , P. Focardi , G. Trinchieri , R. Rampazzo , W. W. Zeilinger

We report the discovery of a large HI cloud in the central regions of the Virgo cluster. It is 110 x 25 kpc in size and contains 3.4 x 10^8 Msol of HI. The morphology and kinematics of this cloud strongly suggest that it consists of HI…

Astrophysics · Physics 2009-11-11 Tom Oosterloo , Jacqueline van Gorkom

ASCA observations of NGC 4636 and a southern region have revealed extended X-ray emission to a radius of about 300 kpc from the galaxy. The symmetric nature of the observed surface brightness around NGC 4636 indicates its association to…

We present deep Halpha+[NII], [SII] (6716,6731A) and [OII] (3726,3729A) images of the highly inclined, actively star--forming SBm galaxy NGC 55, located in the nearby Sculptor Group. Due to its proximity, NGC 55 provides a unique…

Astrophysics · Physics 2009-10-28 Annette M. N. Ferguson , Rosemary F. G. Wyse , J. S. Gallagher

As a result of our statistical study of 540 edge-on galaxies, we present here the images and preliminary statistical analysis of a sub-sample of 60 galaxies, that were selected to be S-type warped spirals. Computing the average volumic…

Astrophysics · Physics 2009-10-31 Vladimir Reshetnikov , Francoise Combes

The halos of elliptical galaxies are faint and difficult to explore, but they contain vital clues to both structure and formation. We present the results of an imaging and spectroscopic survey for planetary nebulae (PNe) in the nearby…

Astrophysics · Physics 2009-11-10 Eric W. Peng , Holland C. Ford , Kenneth C. Freeman

(abridged)We present the observations of the pair of interacting galaxies NGC6285/86 carried out with the 6m SAO RAS telescope by using 1D and 2D spectroscopy. The observations of NGC6286 with a long-slit spectrograph (UAGS) near the…

We present imaging Fabry-Perot observations of Halpha emission in the nearly edge-on spiral galaxy NGC 5775. We have derived a rotation curve and a radial density profile along the major axis by examining position-velocity (PV) diagrams…

Astrophysics · Physics 2009-11-13 G. H. Heald , R. J. Rand , R. A. Benjamin , J. A. Collins , J. Bland-Hawthorn

We present measurements of the Galactic halo's X-ray emission for 110 XMM-Newton sight lines, selected to minimize contamination from solar wind charge exchange emission. We detect emission from few million degree gas on ~4/5 of our sight…

Astrophysics of Galaxies · Physics 2015-06-16 David B. Henley , Robin L. Shelton

We present the detection of an enormous disc of cool neutral hydrogen (HI) gas surrounding the S0 galaxy NGC 612, which hosts one of the nearest powerful radio sources (PKS 0131-36). Using the Australia Telescope Compact Array, we detect…

Aims. The extraplanar stellar populations of highly-inclined disk galaxies IC 2233, IC 5052, NGC 4631 and NGC 5023 are analyzed with the goal to quantify their vertical extent and structure. Methods. Based on the single-star photometry, we…

Astrophysics · Physics 2007-05-23 N. A. Tikhonov , O. A. Galazutdinova , I. O. Drozdovsky

We report on the detection of a stellar halo around NGC 1560, a 10^9 Mo spiral galaxy member of the Maffei group. We obtained deep images in the r and i bands using the 10.4m Gran Telescopio Canarias in a field centered at ~ 3.7 arcmin…

Astrophysics of Galaxies · Physics 2018-07-25 Laura Greggio , Renato Falomo , Riccardo Scarpa

Using imaging that shows four magnitudes of main sequence stars, we have discovered that the Galactic globular cluster NGC 1851 is surrounded by a halo that is visible from the tidal radius of 700 arcsec (41 pc) to more than 4500 arcsec…

Astrophysics of Galaxies · Physics 2015-05-14 Edward W. Olszewski , Abhijit Saha , Patricia Knezek , Annapurni Subramaniam , Thomas de Boer , Patrick Seitzer

We present deep HI 21-cm and optical observations of the face-on spiral galaxy M 83 obtained as part of a project to search for high-velocity clouds (HVCs) in nearby galaxies. Anomalous-velocity neutral gas is detected toward M 83, with…

Astrophysics · Physics 2011-02-11 Eric D. Miller , Joel N. Bregman , Bart P. Wakker

High sensitivity H I observations of the nearby spiral galaxy NGC 2403 obtained with the VLA are presented and discussed. The properties of the extended, differentially rotating H I layer with its H I holes, spiral structure and outer warp…

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

The metallicity of galactic gaseous halos provides insights into accretion and feedback of galaxies. The nearby edge-on galaxy NGC 891 has a multi-component gaseous halo and a background AGN (LQAC 035+042 003) projected 5 kpc above the disk…

Astrophysics of Galaxies · Physics 2019-05-15 Zhijie Qu , Joel N. Bregman , Edmund J. Hodges-Kluck

The nearly face-on SBc galaxy M83 (NGC 5236) was observed for 25 ksec with the ROSAT PSPC. We detected 13 point-like sources in this galaxy, 10 of which were previously unknown. We measured extended X-ray radiation from almost the whole…

Astrophysics · Physics 2007-05-23 M. Ehle , W. Pietsch , R. Beck , U. Klein