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相关论文: Neutral Hydrogen Gas in Interacting Galaxies: The …

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(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…

宇宙学与河外天体物理 · 物理学 2015-05-14 Baerbel S. Koribalski , Angel R. Lopez-Sanchez

We present high spatial resolution 21 cm HI maps of the interacting galaxy pair NGC 7714/7715. We detect a massive (2 x 10**9 M(sun)) HI bridge connecting the galaxies that is parallel to but offset from the stellar bridge. A chain of HII…

天体物理学 · 物理学 2009-10-30 Beverly J. Smith , Curt Struck , Richard W. Pogge

XMM-Newton observations of the starburst galaxy NGC 1511 reveal the presence of a previously unknown extended hot gaseous phase of its ISM, which partly extends out of the disk plane. The emission distribution is asymmetric, being brightest…

天体物理学 · 物理学 2008-11-26 M. Dahlem , M. Ehle , F. Jansen , T. M. Heckman , K. A. Weaver , D. K. Strickland

As part of our study on the impact of violent star formation on the interstellar medium (ISM) of dwarf galaxies, we report observations of neutral atomic hydrogen (HI) in the post-starburst dwarf galaxy NGC 1569. High-resolution…

天体物理学 · 物理学 2008-11-26 S. Muehle , U. Klein , E. M. Wilcots , S. Huettemeister

We present WSRT observations of high sensitivity and resolution of the neutral hydrogen in the starburst dwarf galaxy NGC 1569. Assuming a distance of 2.2 Mpc, we find a total HI mass of 1.3 * 10^8 M_sun to be distributed in the form of a…

天体物理学 · 物理学 2009-11-07 J. M. Stil , F. P. Israel

We present Australia Telescope Compact Array (ATCA) HI imaging of the edge-on galaxy NGC 1596, which was recently found to have counter-rotating ionized gas in its center (<15"). We find a large HI envelope associated with a nearby…

天体物理学 · 物理学 2009-11-11 Aeree Chung , Baerbel Koribalski , Martin Bureau , J. H. van Gorkom

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…

This paper reports on the atomic hydrogen gas (HI) observations of the spiral galaxy NGC 1566 using the newly commissioned Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope. We measure an integrated HI flux density of…

High-sensitivity maps of the large-scale structure of atomic hydrogen in the starburst dwarf galaxy NGC 1569 show evidence for an HI cloud with a mass of 7*10**6 M_sun, at a projected distance of 5 kpc from the parent galaxy. This cloud may…

天体物理学 · 物理学 2007-05-23 J. M. Stil , F. P. Israel

We present new multi-configuration HI aperture synthesis imaging of the nearby dwarf starburst galaxy NGC 625 obtained with the Australia Telescope Compact Array. Total HI column density images show gas well-aligned with the optical major…

天体物理学 · 物理学 2009-11-10 John M. Cannon , N. M. McClure-Griffiths , Evan D. Skillman , Stephanie Cote

We present MeerKAT HI line observations of the nearby interacting galaxy pair NGC 1512/1510. The MeerKAT data yield high-fidelity image sets characterised by an excellent combination of high angular resolution (~20") and and sensitivity…

星系天体物理 · 物理学 2023-09-06 E. Elson , M. Głowacki , R. Deane , N. Isaacs , X. Ndaliso

NGC 2146 is a peculiar spiral galaxy which is currently undergoing a major burst of star formation and is immersed in a extended HI structure that has morphological and kinematical resemblence to a strong tidal interaction. This paper…

天体物理学 · 物理学 2009-10-31 A. Taramopoulos , H. Payne , F. H. Briggs

We present Australia Compact Telescope Array (ATCA) 21-cm observations of the nearby low-excitation radio galaxy (LERG) NGC 3100. This is the brightest galaxy of a loose group and hosts a young ($\sim 2$ Myr) radio source. The ATCA…

星系天体物理 · 物理学 2023-07-05 F. M. Maccagni , I. Ruffa , A. Loni , I. Prandoni , R. Ragusa , D. Kleiner , P. Serra , E. Iodice , M. Spavone

We present UBVJHKHalpha and HI data of the irregular galaxy NGC 2366. It is a normal boxy-shaped disk seen at high inclination angle. We do not see any unambiguous observational signature of a bar. There is an asymmetrical extension of…

天体物理学 · 物理学 2009-11-06 D. A. Hunter , B. G. Elmegreen , H. van Woerden

A mosaic of six HI line observations with the Australia Telescope Compact Array is used to search for intergalactic gas in the NGC 1808 group of galaxies. Within the field of view of about 1.4 deg x 1.2 deg, no emission from intergalactic…

天体物理学 · 物理学 2009-11-06 Michael Dahlem , Matthias Ehle , Stuart D. Ryder

We present results from GMRT HI 21 cm line observations of the interacting galaxy pair Arp 181 (NGC 3212 and NGC 3215) at z =0.032. We find almost all of the detected HI (90%) displaced well beyond the optical disks of the pair with the…

宇宙学与河外天体物理 · 物理学 2015-06-12 Chandreyee Sengupta , K. S. Dwarakanath , D. J. Saikia , T. C. Scott

We present the high-sensitivity and large-scale atomic hydrogen (HI) observations towards lenticular (S0) galaxy NGC 4111 using the Five-hundred-meter Aperture Spherical Radio Telescope (FAST). The column density map shows that NGC4111 and…

星系天体物理 · 物理学 2025-03-10 Mei Ai , Ming Zhu , Nai-ping Yu , Jin-long Xu , Xiao-lan Liu , Yingjie Jing , Qian Jiao , Yao Liu , Chuan-peng Zhang , Jie Wang , Peng Jiang

We present the results of Giant Metrewave Radio Telescope (GMRT) observations of the interacting system Arp86 in both neutral atomic hydrogen, HI, and in radio continuum at 240, 606 and 1394 MHz. In addition to HI emission from the two…

宇宙学与河外天体物理 · 物理学 2015-05-13 Chandreyee Sengupta , K. S. Dwarakanath , D. J. Saikia

A number of very small isolated HII regions have been discovered at projected distances up to 30 kpc from their nearest galaxy. These HII regions appear as tiny emission line objects in narrow band images obtained by the NOAO Survey for…

天体物理学 · 物理学 2015-06-24 E. V. Ryan-Weber , G. R. Meurer , K. C. Freeman , M. E. Putman , R. L. Webster , the SINGG team

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…

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