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相关论文: Unusual displacement of HI due to tidal interactio…

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We present results from our Giant Metrewave Radio Telescope (GMRT) HI observations of the Arp 305 system. The system consists of two interacting spiral galaxies NGC 4016 and NGC 4017, a large amount of resultant tidal debris and a prominent…

星系天体物理 · 物理学 2017-06-28 C. Sengupta , T. C. Scott , S. Paudel , K. S. Dwarakanath , D. J. Saikia , B. W. Sohn

Context: Pre-merger interactions between galaxies can induce significant changes in the morphologies and kinematics of the stellar and ISM components. Large amounts of gas and stars are often found to be disturbed or displaced as tidal…

星系天体物理 · 物理学 2015-12-16 Chandreyee Sengupta , Thomas. C. Scott , Sanjaya Paudel , D. J. Saikia , K. S. Dwarakanath , B. W. Sohn

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

We present results from our Giant Metrewave Radio Telescope (GMRT) HI observations of the interacting pair Arp 202 (NGC 2719 and NGC 2719A). Earlier deep UV(GALEX) observations of this system revealed a tidal tail like extension with a…

星系天体物理 · 物理学 2015-06-22 Chandreyee Sengupta , T. C. Scott , K. S. Dwarakanath , D. J. Saikia , B. W. Sohn

We use the single-dish radio telescope FAST to map the HI in the tidally interacting NGC 4631 group with a resolution of 3.24$'$ (7 kpc), reaching a 5-$\sigma$ column density limit of $10^{17.9}$ cm$^{-2}$ assuming a line width of 20 km…

We present a wide-field, high spatial and velocity resolution map of the entire extended HI distribution of the nearby Local Group dwarf galaxy NGC 6822. The observations were obtained with the Parkes single-dish telescope and the Australia…

天体物理学 · 物理学 2007-05-23 W. J. G. de Blok , F. Walter

We present results from our Giant Metrewave Radio Telescope (GMRT) HI, Himalayan Chandra Telescope (HCT) Halpha, 1m Sampurnanand Telescope (ST) and 1.3m Devasthal Fast Optical Telescope (DFOT) deep optical observations of NGC 7805/6 (Arp…

We report on high-sensitivity neutral hydrogen observations toward the gas-rich interacting galaxies NGC 3395/3396 with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Compared to previous observations carried out by the…

星系天体物理 · 物理学 2024-08-01 Nai-Ping Yu , Ming Zhu , Jin-Long Xu , Chuan-Peng Zhang , Hai-Yang Yu , Xiao-Lan Liu , Peng Jiang , Mei Ai

We present the results of new radio interferometer HI line observations for the merging galaxy pair NGC 4038/9 (`The Antennae'), obtained using the Australia Telescope Compact Array. The results improve substantially on those of van der…

天体物理学 · 物理学 2009-11-06 S. Gordon , B. Koribalski , K. Jones

We present a statistical study of the properties of diffuse HI in ten nearby galaxies, comparing the HI detected by the single-dish telescope FAST (FEASTS program) and the interferometer VLA (THINGS program), respectively. The THINGS'…

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

(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

Among the various phenomena observed in interacting galaxies is the ejection due to tidal forces of material into the intergalactic medium and its subsequent rearranging which can lead to the formation of self-gravitating tidal dwarf…

天体物理学 · 物理学 2014-10-13 P. -A. Duc , E. Brinks , V. Springel , B. Pichardo , P. Weilbacher , I. F. Mirabel

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

We present new optical imaging and spectroscopy and HI spectral line imaging of the dwarf galaxy ADBS 113845+2008 (hereafter ADBS 1138). This metal-poor (Z~30% Z_Sun), "post-starburst" system has one of the most compact stellar…

星系天体物理 · 物理学 2011-02-11 John M. Cannon , John J. Salzer , Jessica L. Rosenberg

We present a wide-field, high spatial and velocity resolution map of the entire extended HI distribution of the Local Group dwarf galaxy NGC 6822. The observations were obtained with the Australia Telescope Compact Array in mosaicing mode.…

天体物理学 · 物理学 2009-10-31 W. J. G. de Blok , F. Walter

We present HI line and 20-cm radio continuum observations of the NGC 1511 galaxy group obtained with the Australia Telescope Compact Array. The data reveal an extended, rather disturbed HI distribution for the peculiar starburst galaxy NGC…

天体物理学 · 物理学 2009-11-10 B. Koribalski , E. Manthey

ATCA HI and radio continuum observations of the peculiar southern galaxy IC2554 and its surroundings reveal typical signatures of an interacting galaxy group. We detected a large HI cloud between IC2554 and the elliptical galaxy NGC3136B.…

天体物理学 · 物理学 2009-11-07 Baerbel Koribalski , Scott Gordon , Keith Jones

We observed the classical interacting galaxy M51 with FAST and obtain high sensitivity HI image with column density down to 3.8 $\times$ 10$^{18}$ cm$^{-2}$. In the image we can see a diffuse extended envelope around the system and several…

星系天体物理 · 物理学 2023-02-15 Haiyang Yu , Ming Zhu , Jin-Long Xu , Mei Ai , Peng Jiang , Yanbin Yang

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
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