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相关论文: Centaurus A: Morphology and kinematics of the HI d…

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We present new observations, performed with the Australia Telescope Compact Array, of the HI absorption in the central regions of Centaurus A. For the first time, absorption is detected against the radio core at velocities blueshifted with…

天体物理学 · 物理学 2009-11-13 R. Morganti , T. Oosterloo , C. Struve , L. Saripalli

We present new ATCA 21-cm line observations of the neutral hydrogen in the nearby radio galaxy Centaurus A. We image in detail (with a resolution down to 7", ~100pc) the distribution of HI along the dust lane. Our data have better velocity…

宇宙学与河外天体物理 · 物理学 2015-05-18 C. Struve , T. A. Oosterloo , R. Morganti , L. Saripalli

New HI observations of the nearby radio-loud galaxies Centaurus A and B2 0258+35 show broad absorption (Delta_v=400km/s) against the unresolved nuclei. Both sources belong to the cases where blue- and redshifted absorption is observed at…

天体物理学 · 物理学 2008-07-29 Christian Struve , Raffaella Morganti , Tom A. Oosterloo

We report on atomic gas (HI) and molecular gas (as traced by CO(2-1)) redshifted absorption features toward the nuclear regions of the closest powerful radio galaxy, Centaurus A (NGC 5128). Our HI observations using the Very Long Baseline…

宇宙学与河外天体物理 · 物理学 2015-05-19 D. Espada , A. B. Peck , S. Matsushita , K. Sakamoto , C. Henkel , D. Iono , F. P. Israel , S. Muller , G. Petitpas , Y. Pihlstroem , G. B. Taylor , D. V. Trung

Due to the proximity, the neutral hydrogen belonging to Centaurus A can be observed at high resolution with good sensitivity. This allows to study the morphology and kinematics in detail in order to understand the evolution of this…

宇宙学与河外天体物理 · 物理学 2015-05-14 Christian Struve , Raffaella Morganti , Tom A. Oosterloo , Bjorn H. C. Emonts

Centaurus A, the nearest AGN shows molecular absorption in the millimeter and radio regime. By observing the absorption with VLBI, we try to constrain the distribution of the gas, in particular whether it resides in the circumnuclear…

天体物理学 · 物理学 2009-11-10 H. J. van Langevelde , Y. Pihlstroem , A. Beasley

We present Very Long Baseline Array (VLBA) HI absorption observations of the core region of the powerful radio galaxy Cygnus A. These data show both broad (FWHM = 231 \pm 21 km/s) and narrow (FWHM <30 km/s) velocity width absorption…

宇宙学与河外天体物理 · 物理学 2015-05-14 Christian Struve , John E. Conway

We present new 21-cm HI observations performed with ATCA of the large HI filament located about 15 kpc NE from the centre of Centaurus A and discovered by Schiminovich et al.(1994). This HI cloud is situated (in projection) near the radio…

天体物理学 · 物理学 2009-11-10 T. A. Oosterloo , R. Morganti

We compile position and inclination angles for tilted ring fits to the warped dusty and gaseous disk spanning radius 1.8 to 6500 pc from recent observations. For radii exterior to a kpc, tilted ring orientations lie on an arc on a polar…

星系天体物理 · 物理学 2015-05-14 Alice C. Quillen , Nadine Neumayer , Tom Oosterloo , Daniel Espada

We have observed Centaurus A with the MID-infrared Interferometric instrument (MIDI) at the Very Large Telescope Interferometer (VLTI) at resolutions of 7 - 15 mas (at 12.5 micron) and filled gaps in the (u,v) coverage in comparison to…

宇宙学与河外天体物理 · 物理学 2010-10-18 Leonard Burtscher , Klaus Meisenheimer , Walter Jaffe , Konrad R. W. Tristram , Huub J. A. Röttgering

This review summarizes the state of the knowledge of the nearby (D = 3.4 Mpc) radio source Centaurus A and its host galaxy NGC 5128. The massive elliptical host galaxy appears to be moderately triaxial. It contains a strongly warped thin…

天体物理学 · 物理学 2009-10-31 F. P. Israel

Spitzer mid-infrared images of the dusty warped disk in the galaxy Centaurus A show a parallelogram-shaped structure. We successfully model the observed mid-infrared morphology by integrating the light from an emitting, thin, and warped…

Forward asteroseismic modelling plays an important role towards a complete understanding of the physics taking place in deep stellar interiors. With a dynamical mass in the range over which models develop convective cores while in the main…

太阳与恒星天体物理 · 物理学 2019-04-25 Benard Nsamba , Tiago L. Campante , Mário J. P. F. G. Monteiro , Margarida S. Cunha , Sérgio G. Sousa

We present two-dimensional gas-kinematic maps of the central region in Centaurus A. The adaptive optics (AO) assisted SINFONI data from the VLT have a resolution of 0.12" in K-band. The ionized gas species (Br_gamma, [FeII], [SiVI]) show a…

天体物理学 · 物理学 2009-11-13 N. Neumayer , M. Cappellari , J. Reunanen , H. -W. Rix , P. P. van der Werf , P. T. de Zeeuw , R. I. Davies

VLA observations of large-scale HI and OH absorption in the merging galaxy of NGC6240 are presented with 1 arcsec resolution. HI absorption is found across large areas of the extended radio continuum structure with a strong concentration…

天体物理学 · 物理学 2011-02-11 Willem A. Baan , Yoshiaki Hagiwara , Peter Hofner

We present WSRT and VLA radio observations of the neutral hydrogen in the radio galaxy Coma A. We detect extended HI absorption against both radio lobes of Coma A, at distances of about 30 kpc from the centre. Coma A is the first radio…

天体物理学 · 物理学 2009-11-07 R. Morganti , T. A. Oosterloo , S. Tinti , C. N. Tadhunter , K. A. Wills , G. van Moorsel

We used the near infrared spectrometer ISAAC at the ESO 'Very Large Telescope' to map the velocity field of Centaurus A (NGC 5128) at several position angles and locations in the central 20" of the galaxy. The high spatial resolution…

We report new HST WFPC2 and NICMOS observations of the center of the nearest radio galaxy Centaurus A (NGC 5128) and discuss their implications for our understanding of the active nucleus and jet. We detect the active nucleus in the near-IR…

We present high resolution images of the 12CO(2-1) emission in the central 1' (1 kpc) of NGC 5128 (Centaurus A), observed using the SMA. We elucidate for the first time the distribution and kinematics of the molecular gas in this region…

We present results from a sensitive high-resolution X-ray observation of the nearby active galaxy Centaurus A (NGC 5128) with the ROSAT HRI. The 65~ksec X-ray image clearly distinguishes different components of the X-ray emission from Cen…

天体物理学 · 物理学 2009-10-28 S. Doebereiner , N. Junkes , S. J. Wagner , H. Zinnecker , R. Fosbury , G. Fabbiano , E. J. Schreier
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