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相关论文: AGC 226067: A possible interacting low-mass system

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Observations with the Green Bank Telescope of 21cm HI emission from the high-velocity cloud Complex H suggest that it is interacting with the Milky Way. A model in which the cloud is a satellite of the Galaxy in an inclined, retrograde…

天体物理学 · 物理学 2009-11-07 Felix J. Lockman

We describe the properties of a remarkable group of actively star-forming dwarf galaxies and HII galaxies in the Abell 1367 cluster, which were discovered in a large-scale H-alpha imaging survey of the cluster. Approximately 30…

天体物理学 · 物理学 2009-11-07 Shoko Sakai , Robert Kennicutt , J. M. van der Hulst , Chris Moss

We present the results of a 21 cm neutral hydrogen (HI) line detection experiment in the direction of 18 low luminosity dwarf galaxies of the Centaurus A group, using the Australia Telescope National Facility 64m Parkes Radio Telescope and…

天体物理学 · 物理学 2008-11-26 A. Bouchard , H. Jerjen , G. S. Da Costa , J. Ott

As part of the HI Arecibo Galaxy Environments Survey (AGES) we have observed 5$\times$4 degrees of sky centred on M33, reaching a limiting column density of $\sim 1.5 \times 10^{17}$ cm$^{-2}$ (line width of 10 km s$^{-1}$ and resolution…

星系天体物理 · 物理学 2016-01-13 Olivia Keenan , Jonathan Davies , Rhys Taylor , Robert Minchin

Radio observations of gas in the Milky Way and Local Group are vital for understanding how galaxies function as systems. The unique sensitivity of Arecibo's 305m dish, coupled with the 7-beam Arecibo L-Band Feed Array (ALFA), provides an…

天体物理学 · 物理学 2009-06-23 S. J. Gibson , K. A. Douglas , C. Heiles , E. J. Korpela , J. E. G. Peek , M. E. Putman , S. Stanimirović

We present a photometric study of UGC 4599, a low-luminosity galaxy superficially resembling Hoag's Object in that on sky survey images it appears to be a complete ring surrounding a roundish core. The nature of the outer ring of Hoag-type…

宇宙学与河外天体物理 · 物理学 2015-05-27 Ido Finkelman , Noah Brosch

We present preliminary results of VLA HI imaging of selected Virgo cluster galaxies. The goal is to study environmental effects on galaxy evolution. Our sample of 41 galaxies is spread throughout the cluster and spans a wide range in star…

天体物理学 · 物理学 2007-05-23 Aeree Chung , J. H. van Gorkom , Jeffery D. P. Kenney , Bernd Vollmer

Using long-slit optical spectra obtained with the 2-m telescope at IUCAA Girawali Observatory, we show that the radio source J094221.98+062335.2 (z=0.123) is associated with a galaxy pair undergoing a major merger. Its companion is a normal…

星系天体物理 · 物理学 2015-08-06 R. Srianand , N. Gupta , E. Momjian , M. Vivek

We investigate the global neutral hydrogen (HI) content of isolated galaxies selected from the SDSS spectroscopic survey with optical evidence of Active Galactic Nuclei (AGN). Our sample includes galaxies with unresolved HI observations…

星系天体物理 · 物理学 2018-07-18 Jeremy D. Bradford , Marla C. Geha , Jenny E. Greene , Amy E. Reines , Claire M. Dickey

The nearby galaxy HIZSS003 was recently discovered during a blind HI survey of the zone of avoidance (Henning et al. 2000). Follow up VLA as well as optical and near-IR imaging and spectroscopy (Massey et al. 2003; Silva et al. 2005)…

天体物理学 · 物理学 2009-11-10 Ayesha Begum , Jayaram N. Chengalur , I. D. Karachentsev , M. E. Sharina

A deep HST image of the MS 2137-2353 core has revealed detailed morphological structures in two arc systems, which are modelled and well reproduced after a complete analysis of the lensing properties of the dark matter component. Latter…

天体物理学 · 物理学 2007-05-23 F. Hammer , P. Teyssandier , E. J. Shaya , I. M. Gioia , G. A. Luppino , O. Le Fèvre

We have identified a new group of galaxies, CG J0247+44.9, at low Galactic latitude (l=143.64 deg, b=-13.29 deg), which satisfies Hickson's criteria (Hickson 1997) for Compact Groups (CGs). Our group consists of six members, two of which…

天体物理学 · 物理学 2009-11-07 Sonia Temporin , Stefano Ciroi

Our GMRT HI observations of the ultra diffuse galaxy (UDG) UGC 2162, projected $\sim$ 300 kpc from the centre of the M77 group, reveal it to a have an extended HI disk (R$_{HI}$/R$_{25}$ $\sim$ 3.3) with a moderate rotational velocity…

星系天体物理 · 物理学 2019-07-31 Chandreyee Sengupta , T. C. Scott , Aeree Chung , O. Ivy Wong

Here, we present a kinematical analysis of the Virgo cluster ultra-diffuse galaxy (UDG) VCC 1287 based on data taken with the Keck Cosmic Web Imager (KCWI). We confirm VCC 1287's association both with the Virgo cluster and its globular…

We investigate the dwarf (M_B> -16) galaxies in the Virgo cluster in the radio, optical, and ultraviolet regimes. Of the 365 galaxies in this sample, 80 have been detected in HI by the Arecibo Legacy Fast ALFA survey. These detections…

We present Giant Metrewave Radio Telescope (GMRT) HI 21-cm line data for the smallest known eXtremely Metal Deficient (XMD) blue compact galaxy (BCG) HS0822+3542. From HST imaging it has been suggested that HS0822+3542 actually consists of…

天体物理学 · 物理学 2007-05-23 Jayaram N. Chengalur , S. A. Pustilnik , J. -M. Martin , A. Y. Kniazev

Based on 14 data points obtained with near-infrared speckle interferometry and covering an almost entire revolution, we present a first visual orbit for the low-mass binary system Gliese 22 AC. The quality of the orbit is largely improved…

天体物理学 · 物理学 2009-11-07 J. Woitas , V. S. Tamazian , J. A. Docobo , Ch. Leinert

On the periphery of galaxy clusters, moderately high galaxy densities and velocity dispersions favour interactions and mergers that influence galaxy evolution prior to cluster infall. Observational studies of this phase in dwarfs remain…

We present the detection of a low surface-brightness stellar counterpart to an enormous (190 kpc) ring of neutral hydrogen (HI) gas that surrounds the nearby radio galaxy B2 0648+27. This system is currently in an evolutionary stage between…

天体物理学 · 物理学 2009-11-13 B. H. C. Emonts , R. Morganti , J. H. van Gorkom , T. A. Oosterloo , E. Brogt , C. N. Tadhunter

We report the discovery of four groups of galaxies along the line of sight to the B1608+656 gravitational lens system. One group is at the redshift of the primary lensing galaxy (z = 0.631) and appears to have a low mass, with eight…

天体物理学 · 物理学 2009-11-13 C. D. Fassnacht , R. R. Gal , L. M. Lubin , J. P. McKean , G. K. Squires , A. C. S. Readhead