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Related papers: Gas Dynamics in the Barred Seyfert Galaxy NGC4151 …

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We present sensitive, high resolution observations of neutral hydrogen (HI) in the unusually gas-rich, oval distortion of the Seyfert galaxy NGC4151. The gas dynamics of the oval are found to be consistent with those of a kinematically weak…

Astrophysics · Physics 2009-10-31 C. G. Mundell , D. L. Shone

We have determined the structure and kinematics of ionised gas in the weak oval bar of the archetypal Seyfert 1 galaxy, NGC 4151, using the TAURUS Fabry-Perot interferometer to simultaneously map the distribution and kinematics of Hbeta…

Astrophysics · Physics 2009-11-10 M. W. Asif , C. G. Mundell , A. Pedlar

Sensitive high angular and linear resolution radio images of the 240-pc radio jet in NGC4151, imaged at linear resolutions of 0.3 to 2.6 pc using the VLBA and phased VLA at 21 cm, are presented and reveal for the first time a faint, highly…

Astrophysics · Physics 2011-09-30 C. G. Mundell , J. M. Wrobel , A. Pedlar , J. F. Gallimore

We present a detailed analysis of the intrinsic X-ray absorption in the Seyfert 1 galaxy NGC 4151 using Chandra/HETGS data obtained 2002 May, as part of a program which included simultaneous UV spectra using HST/STIS and FUSE. NGC 4151 was…

We observed the Seyfert 1 galaxy NGC 4151 on eleven occasions at 1-2 day intervals using the Berkeley spectrometer during the ORFEUS-SPAS II mission in 1996 November. The mean spectrum covers 912-1220 A at ~0.3 A resolution with a total…

Astrophysics · Physics 2009-10-30 B. R. Espey , G. A. Kriss , J. H. Krolik , W. Zheng , Z. Tsvetanov , A. F. Davidsen

Active galaxies are thought to be both fueled and obscured by neutral gas removed from the host galaxy and funneled into a central accretion disk. We performed a VLA imaging survey of 21 cm absorption in Seyfert and starburst nuclei to…

Astrophysics · Physics 2009-10-31 J. F. Gallimore , S. A. Baum , C. P. O'Dea , A. Pedlar , E. Brinks

The first detailed VLA mapping of the neutral hydrogen distribution in the isolated, edge-on spiral galaxy NGC 3044 is presented. Physical parameters determined for this galaxy are typical for galaxies of its morphological class (SBc). We…

Astrophysics · Physics 2009-10-30 Siow-Wang Lee , Judith A. Irwin

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 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…

Astrophysics · Physics 2009-11-06 D. A. Hunter , B. G. Elmegreen , H. van Woerden

We have examined the physical conditions in intrinsic UV-absorbing gas in the Seyfert galaxy NGC 4151, using echelle spectra obtained with the Space Telescope Imaging Spectrograph (STIS). We confirm the presence of the kinematic components…

The Seyfert 1 galaxy NGC4151 is characterized by complex X-ray absorption, well described by a dual absorber, composed of a uniform mildly ionized gas and a cold system that partially covers the central source. However, in one of the 5…

Astrophysics · Physics 2009-11-11 L. Piro , A. De Rosa , G. Matt , G. C. Perola

Images at 12.5 microns of nuclei of three nearby Seyfert galaxies -- NGC 1275, NGC 4151 and NGC 7469 -- have been obtained with the Keck 10-m Telescope. NGC 7469 is resolved and deconvolution delineates a structure <0.04"x0.08" or <13x26 pc…

Astrophysics · Physics 2009-11-07 B. T. Soifer , J. J. Bock , K. Marsh , G. Neugebauer , K. Matthews , E. Egami , L. Armus

We present preliminary results from a study of the neutral hydrogen (HI) properties of an X-ray selected sample of nearby loose galaxy groups. This forms part of a multi-wavelength investigation (X-ray, optical and radio) of the formation…

Astrophysics · Physics 2007-05-23 N. P. F. McKay , C. G. Mundell , S. Brough , D. A. Forbes , D. G. Barnes

We have used the Gemini Near-infrared Integral Field Spectrograph (NIFS) to map the emission-line intensity distributions and ratios in the Narrow-Line Region (NLR) of the Seyfert galaxy NGC 4151 in the Z, J, H and K bands at a resolving…

We have used the Gemini NIFS to map the gas kinematics of the inner 200x500pc of the Seyfert galaxy NGC4151 in the Z, J, H and K bands at a resolving power 5000 and spatial resolution of 8pc. The ionised gas emission is most extended along…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-14 T. Storchi-Bergmann , R. D. Simões-Lopes , P. J. McGregor , Rogemar A. Riffel , T. Beck , P. Martini

We present the Chandra discovery of soft diffuse X-ray emission in NGC 4151 (L[0.5-2keV]~10^{39} erg s$^{-1}$), extending ~2 kpc from the active nucleus and filling in the cavity of the HI material. The best fit to the X-ray spectrum…

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…

Astrophysics of Galaxies · Physics 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 ISO-SWS and ISOPHOT-S spectroscopy of the Seyfert galaxy NGC 4151. We detect a total of 17 fine structure emission lines emitted by a wide range of low- and high-excitation ions, two rotational lines of molecular hydrogen, and…

Astrophysics · Physics 2016-08-30 E. Sturm , T. Alexander , D. Lutz , A. Sternberg , H. Netzer , R. Genzel

The VLA has been used to image HI in a heterogeneous sample of nine Seyferts as part of a continuing investigation of the role of galactic host gas in the triggering and fuelling of nuclear activity. Where previous single-dish observations…

Astrophysics · Physics 2007-05-23 C. G. Mundell

A detailed kinematic analysis of ionized gas in the nearby irregular galaxy NGC 4449 is presented. Observations are conducted in the spectral lines of Halpha and [SII]. Our scanning Fabry--Perot interferometric observations are presented…

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