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相关论文: Rotational Dynamics and Star Formation in the Near…

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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

NGC 5291, an early-type galaxy surrounded by a giant HI ring, is believed to be formed from collision with another galaxy. Several star forming complexes and tidal dwarf galaxies are distributed along the collisional ring which are sites of…

We present new low-resolution HI spectral line imaging, obtained with the Karl G. Jansky Very Large Array (JVLA), of the star-forming Magellanic irregular galaxy UGCA 105. This nearby (D = 3.39+/-0.25 Mpc), low mass [M_HI=(4.3+/-0.5)x10^8…

We have used the VLA to image the HI 21-cm line emission in the edge-on Sd galaxy IC2233 and the blue compact dwarf NGC2537. We also present new optical B,R, and H alpha imaging of IC2233 obtained with the WIYN telescope. Despite evidence…

天体物理学 · 物理学 2008-11-26 Lynn D. Matthews , Juan M. Uson

Context: High-mass stars have a high degree of multiplicity and most likely form via disk accretion processes. The detailed physics of the binary and disk formation are still poorly constrained. Methods: Using the VLA in its most extended…

太阳与恒星天体物理 · 物理学 2017-09-13 H. Beuther , H. Linz , Th. Henning , S. Feng , R. Teague

Star formation (SF) takes place in unusual places such as way out in the intergalactic medium out of material expelled from parent galaxies. We wish to answer whether SF proceeds in this specific environment in a similar way than in…

天体物理学 · 物理学 2009-11-13 M. Boquien , P. -A. Duc , J. Braine , E. Brinks , U. Lisenfeld , V. Charmandaris

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

I present sensitive high resolution HI VLA B+C+D array observations of the edge-on Scd galaxy NGC 4244. The gas layer of NGC 4244 is rather symmetric in all respects, i.e. the surface density distribution, flaring and warping, so that the…

天体物理学 · 物理学 2009-10-28 Rob P. Olling

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 the first HI spectral line images of the nearby, star-forming dwarf galaxies UGC11411 and UGC 8245, acquired as part of the "Observing for University Classes" program with the Karl G. Jansky Very Large Array (VLA). These…

We investigate the dynamics of starbursting dwarf galaxies, using both new and archival HI observations. We consider 18 nearby galaxies that have been resolved into single stars by HST observations, providing their star formation history…

星系天体物理 · 物理学 2014-06-23 Federico Lelli , Marc Verheijen , Filippo Fraternali

Owing to their shallow stellar potential, dwarf galaxies possess thick gas disks, which makes them good candidates for studies of the galactic vertical kinematical structure. We present 21 cm line observations of the isolated nearby dwarf…

Abridged. Context. The metal content of dwarf galaxies and the metal enrichment of the intergalactic medium both suggest that mass loss from galaxies is a significant factor for the chemical evolution history of galaxies, in particular of…

天体物理学 · 物理学 2009-11-13 J. van Eymeren , M. Marcelin , B. Koribalski , R. -J. Dettmar , D. J. Bomans , J. -L. Gach , P. Balard

We present a study of the HI distribution and dynamics of the nearby spiral galaxy NGC5055 based on observations with the Westerbork Synthesis Radio Telescope. The gaseous disk of NGC5055 extends out to about 40 kpc, equal to 3.5 R_25, and…

天体物理学 · 物理学 2009-11-11 G. Battaglia , F. Fraternali , T. Oosterloo , R. Sancisi

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

We report a new high-sensitivity HI mapping observation of the NGC 5055 galaxy group over an area of $1.^\circ5\times0.^\circ75$ with the Five-hundred-meter Aperture Spherical radio Telescope (FAST). Our observation reveals that the warped…

星系天体物理 · 物理学 2024-10-01 Xiao-Lan Liu , Ming Zhu , Jin-Long Xu , Peng Jiang , Chuan-Peng Zhang , Nai-Ping Yu , Jun-Jie Wang , Yan-Bin Yang

We present observations of the nuclear star cluster in the nearby edge-on spiral galaxy NGC 4244 using the Gemini Near-Infrared Integral Field Spectrograph (NIFS) with laser guide star adaptive optics. From a previous study of edge-on…

Context. Outflows powered by the injection of kinetic energy from massive stars can strongly affect the chemical evolution of galaxies, in particular of dwarf galaxies, as their lower gravitational potentials enhance the chance of a…

宇宙学与河外天体物理 · 物理学 2015-05-13 J. van Eymeren , M. Marcelin , B. S. Koribalski , R. -J. Dettmar , D. J. Bomans , J. -L. Gach , P. Balard

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…

天体物理学 · 物理学 2008-11-26 P. N. Appleton , V. Charmandaris , Yu Gao , T. Jarrett , M. A. Bransford
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