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We present new radio observations of the brighter region of the northern lobe (the Northern Middle Lobe, NML) of Centaurus A obtained at 20 cm with the Australia Telescope Compact Array. The angular resolutions are ~50 and ~130 arcsec,…

Astrophysics · Physics 2009-10-31 R. Morganti , N. E. B. Killeen , R. D. Ekers , T. A. Oosterloo

We have carried out the harmonic analysis of the atomic hydrogen (HI) surface density maps and the velocity fields for 11 galaxies belonging to the Ursa Major group, over a radial range of 4-6 disc scalelengths in each galaxy. This analysis…

Astrophysics · Physics 2008-11-26 R. A. Angiras , C. J. Jog , K. S. Dwarakanath , M. A. W. Verheijen

We present J, H and K-band images and 0.9-2.5 micron spectra of the nuclear regions of Centaurus A obtained with IRIS on the AAT. While K band has a point source coincident with the nucleus, at H and J we identify diffuse structure…

Astrophysics · Physics 2009-10-31 J. J. Bryant , R. W. Hunstead

We present new radio continuum, 21 cm HI, and 2.6 mm CO data for the peculiar radio galaxy NGC 4410A and its companion NGC 4410B, and compare with available optical and X-ray maps. Our radio continuum maps show an asymmetric…

Astrophysics · Physics 2009-10-31 Beverly J. Smith

Centaurus A is the closest radio-loud active galaxy. Very Long Baseline Interferometry (VLBI) enables us to study the jet-counterjet system on milliarcsecond (mas) scales, providing essential information for jet emission and propagation…

We study the multi-phase medium in the vicinity of the active galactic nucleus Centaurus A (Cen A). Combined high-resolution observations with the ALMA and Chandra observatories indicate that the hot X-ray emitting plasma coexists with the…

Astrophysics of Galaxies · Physics 2020-11-25 A. Borkar , T. P. Adhikari , A. Różańska , A. G. Markowitz , P. G. Boorman , B. Czerny , G. Migliori , B. De Marco , V. Karas

We present results of a study of neutral hydrogen (HI) in a complete sample of nearby non-cluster radio galaxies. We find that radio galaxies with large amounts of extended HI (M_HI >= 10^9 M_solar) all have a compact radio source. The host…

NGC 3311, the central galaxy of the Hydra I cluster, shows signatures of recent infall of satellite galaxies from the cluster environment. Previous work has shown that the line-of-sight velocity dispersion of the stars and globular clusters…

Astrophysics of Galaxies · Physics 2018-11-14 M. Hilker , T. Richtler , C. E. Barbosa , M. Arnaboldi , L. Coccato , C. Mendes de Oliveira

We report observations at mid-infrared and sub-millimeter wavelengths of Centaurus A (CenA, NGC 5128), the giant elliptical galaxy that harbors the closest radio loud Active Galactic Nucleus (AGN) to Earth. The dust emission from the deep…

We present the first results of a study aimed to detect large HI structures in radio galaxies. In two of the three cases presented (Coma A and B2 0648+27), the detection of a large amount of HI distributed over several tens of kpc suggests…

Astrophysics · Physics 2009-11-07 R. Morganti , T. Oosterloo , C. Tadhunter , B. Emonts

NGC 5128 is one of the best targets to study AGN-feedback in the local Universe. At 13.5 kpc from the galaxy, optical filaments with recent star formation lie along the radio-jet direction. It is a testbed region for positive feedback…

We present new results on the shock around the southwest radio lobe of Centaurus A using data from the Chandra Very Large Programme observations. The X-ray spectrum of the emission around the outer southwestern edge of the lobe is well…

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…

Astrophysics of Galaxies · Physics 2015-08-06 R. Srianand , N. Gupta , E. Momjian , M. Vivek

Supermassive black holes and supernovae explosions at the centres of active galaxies power cycles of outflowing and inflowing gas that affect galactic evolution and the overall structure of the Universe. While simulations and observations…

We report SMA 335 GHz continuum observations with angular resolution of ~0.''3, together with VLA ammonia observations with ~1'' resolution toward Cep A HW 2. We find that the flattened disk structure of the dust emission observed by Patel…

Astrophysics · Physics 2009-11-13 J. M. Torrelles , N. A. Patel , S. Curiel , P. T. P. Ho , G. Garay , L. F. Rodriguez

We investigate the physical structure of the gas component of the disk around the pre-main-sequence star HD169142. The 13CO and C18O J=2-1 line emission is observed from the disk with 1.4'' resolution using the Submillimeter Array. We adopt…

Astrophysics · Physics 2008-06-12 Olja Panić , Michiel R. Hogerheijde , David Wilner , Chunhua Qi

We report HST NICMOS observations of the central region of NGC 5128 at 2.2mic and in Paschen Alpha (PA). The continuum images show extended emission typical of an elliptical galaxy and a strong unresolved central source we identify as the…

We investigate signatures of a jet-interstellar medium (ISM) interaction using optical integral-field observations of the so-called outer filament near Centaurus A, expanding on previous results obtained on a more limited area. Using the…

Astrophysics of Galaxies · Physics 2015-02-18 F. Santoro , J. B. R. Oonk , R. Morganti , T. A. Oosterloo , G. Tremblay

We examine the gas kinematics of the LMC revealed by the high spatial and velocity resolution HI data cube of the combined ATCA and Parkes telescope surveys. We adopt an approach designed to facilitate comparisons with quasar absorption…

Astrophysics · Physics 2009-11-07 Jason X. Prochaska , Emma Ryan-Weber , Lister Staveley-Smith