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相关论文: HI Spatial Distribution in the Galaxy NGC 3783

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We have conducted wide-field HI mapping of a ~5.5 x 5.5 degree region surrounding the NGC 3783 galaxy group, to an HI mass limit of ~4 x 10^8 Msun. The observations were made using the multibeam system on the Parkes 64-m radiotelescope, as…

天体物理学 · 物理学 2009-11-11 Virginia A. Kilborn , Duncan A. Forbes , Baerbel S. Koribalski , Sarah Brough , Katie Kern

VLA and Parkes 64 m radiotelescope 21-cm observations of the starburst dwarf galaxy NGC 5253 reveal a multi-component non-axisymmetric HI distribution. The component associated with the stellar body shows evidence for a small amount of…

天体物理学 · 物理学 2009-11-13 Henry A. Kobulnicky , Evan. D. Skillman

Neutral hydrogen observations of the nearby, edge-on spiral galaxy NGC 891 reveal the presence of an HI halo extending up to at least 5 kpc from the plane. This halo gas appears to rotate 25 to 100 km/s more slowly than the gas in the…

天体物理学 · 物理学 2009-05-29 R. A. Swaters , R. Sancisi , J. M. van der Hulst

VLA neutral hydrogen observations of the shell elliptical NGC 3656 reveal an edge-on, warped minor axis gaseous disk (M_HI ~ 2.10^9 Msun) extending 7 kpc. HI is also found outside the optical image, on two complexes to the North-East and…

天体物理学 · 物理学 2009-11-06 M. Balcells , J. H. van Gorkom , R. Sancisi , C. del Burgo

New high resolution, high sensitivity WSRT HI synthesis observations of the spiral galaxy NGC 3631 are presented. In the total atomic hydrogen map, the spiral arms are well distinguished from the interarm regions, while the sensitivity…

天体物理学 · 物理学 2015-06-24 J. H. Knapen

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

We have analyzed high velocity resolution HI synthesis observations of the nearly face-on Sc galaxy NGC 1232. The neutral gas distribution extends well beyond the optical extent of the galaxy. As expected, local peaks in the HI column…

天体物理学 · 物理学 2009-10-31 L. van Zee , J. Bryant

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

Aims: We derive the 3-D HI volume density distribution for the Galactic disk out to R = 60 kpc. Methods: Our analysis is based on parameters for the warp and rotation curve derived previously. The data are taken from the…

天体物理学 · 物理学 2015-05-13 P. M. W. Kalberla , L. Dedes

We model the observed vertical distribution of the neutral hydrogen (HI) in the faint (M_B ~ -13.7 mag) edge-on dwarf irregular galaxy KK250. Our model assumes that the galaxy consists of axi-symmetric, co-planar gas and stellar discs in…

星系天体物理 · 物理学 2014-11-18 Narendra Nath Patra , Arunima Banerjee , Jayaram N. Chengalur , Ayesha Begum

Observations of the neutral atomic hydrogen (HI) in the nuclear starburst galaxy NGC 4945 with MeerKAT are presented. We find a large amount of halo gas, previously missed by HI observations, accounting for 6.8% of the total HI mass. This…

We present excellent resolution and high sensitivity Very Large Array (VLA) observations of the 21cm HI line emission from the face-on galaxy NGC 1058, providing the first reliable study of the HI profile shapes throughout the entire disk…

天体物理学 · 物理学 2009-06-23 A. O. Petric , M. P. Rupen

We present 21-cm observations and models of the neutral hydrogen in NGC 4565, a nearby, edge-on spiral galaxy, as part of the Westerbork Hydrogen Accretion in LOcal GAlaxieS (HALOGAS) survey. These models provide insight concerning both the…

星系天体物理 · 物理学 2015-06-11 Laura K. Zschaechner , Richard J. Rand , George H. Heald , Gianfranco Gentile , Gyula Jòzsa

[Abridged] We present a new deep 21-cm survey of the Andromeda galaxy, based on high resolution observations performed with the Synthesis Telescope and the 26-m antenna at DRAO. The HI distribution and kinematics of the disc are analyzed…

宇宙学与河外天体物理 · 物理学 2014-11-20 Laurent Chemin , Claude Carignan , Tyler Foster

We report the detection of 21-cm line emission from H I in the planetary nebula NGC 7293 (the Helix). The observations, made with the Very Large Array, show the presence of a ring of atomic hydrogen that is associated with the outer portion…

天体物理学 · 物理学 2009-11-07 Luis F. Rodriguez , W. M. Goss , Robert Williams

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…

天体物理学 · 物理学 2007-05-23 Renzo Sancisi , Filippo Fraternali , Tom Oosterloo , Gustaaf van Moorsel

A new deep HI survey of the galaxy Messier 33 is presented, based on observations obtained at the Dominion Radio Astrophysical Observatory. We observe a perturbed outer gas distribution and kinematics in M33, and confirm the disk warping as…

星系天体物理 · 物理学 2017-06-15 S. Zacharie Kam , Claude Carignan , Laurent Chemin , Tyler Foster , Ed Elson , Tom H. Jarrett

We use observations of the neutral atomic hydrogen (HI) 21-cm emission line to study the spatial distribution of the HI gas in a 80$\degree\times~$90$\degree$ region of the Galaxy halo. The HI column densities in the range of…

星系天体物理 · 物理学 2017-09-20 Ericson López , Jairo Armijos , Mario Llerena , Franklin Aldás

We present Australia Telescope Compact Array mosaic HI imaging of the Local Group dwarf irregular galaxy WLM. We find an integrated flux of 149 Jy km/s and a total HI mass of 3.2 x 10^7 solar masses. The major axis of the HI is aligned with…

天体物理学 · 物理学 2009-11-10 Dale C. Jackson , Evan D. Skillman , John M. Cannon , Stephanie Cote

A study is presented of HI line observations of the nearby spiral galaxy NGC 3521 observed with the VLA as part of The HI Nearby Galaxy Survey. Clearly evident in the HI data cube is the presence of an anomalous HI component that is both…

星系天体物理 · 物理学 2013-12-10 Edward Elson
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