activity
20072013
most citedCentaurus A: morphology and kinematics of the atomic hydrogen

76 citations · 358 across the 15 of their papers we have counts for

collaborators

14 papers

astro-ph.CO2013★ 17 cited

Star Formation in Two Luminous Spiral Galaxies

Deidre A. Hunter, Bruce G. Elmegreen, Vera C. Rubin +4

We have examined star formation in two very luminous (M_V=-22 to -23) Sc-type spiral galaxies, NGC 801 and UGC 2885, using ultra-deep Halpha images. We combine these with UBV and 2…

astro-ph.CO2012★ 62 cited

Recurrent radio emission and gas supply: the case of the radio galaxy B2 0258+35

Aleksandar Shulevski, Raffaella Morganti, Tom Oosterloo +1

Outlined is the discovery of a very faint, diffuse, low surface-brightness (0.5 \mJybeam, 1.4 \mJyarcminsq on average) structure around the radio source B2 0258+35 hosted by an HI-…

astro-ph.CO2011★ 7 cited

Classical radio source propagating into outer HI disc in NGC 3801

Bjorn Emonts, Criag Burnett, Raffaella Morganti +1

We present observations of a large-scale disc of neutral hydrogen (HI) in the nearby Fanaroff & Riley type-I radio galaxy NGC 3801 with the Westerbork Synthesis Radio Telescope. Th…

astro-ph.CO2011★ 27 cited

Herschel observations of Cen A: stellar heating of two extragalactic dust clouds

R. Auld, M. W. L. Smith, G. Bendo +18

We present the first results of a multi-wavelength survey, incoporating Herschel-SPIRE, Spitzer, GALEX and ATCA observations, of a 1 deg x 1 deg field centred on Centaurus A. As we…

astro-ph.CO2010★ 44 cited

Cold gas in massive early-type galaxies: The case of NGC 1167

C. Struve, T. A. Oosterloo, R. Sancisi +2

We present a study of the morphology and kinematics of the neutral hydrogen in the gas-rich (M_HI=1.5x10^{10}Msun), massive early-type galaxy NGC 1167, which was observed with the…

astro-ph.CO2010★ 76 cited

Centaurus A: morphology and kinematics of the atomic hydrogen

C. Struve, T. A. Oosterloo, R. Morganti +1

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 distributi…