activity
20032018
most citedA dust component 2 kpc above the plane in NGC 891

37 citations · 113 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2018★ 9 cited

Near-identical star formation rate densities from H and FUV at redshift zero

Fiona M. Audcent-Ross, Gerhardt R. Meurer, O. I. Wong +27

For the first time both H and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: )…

astro-ph.GA2016★ 13 cited

The Shape of Dark Matter Haloes III. Kinematics and Structure of the HI disc

S. P. C. Peters, P. C. van der Kruit, R. J. Allen +1

We present a new strategy for fitting the structure and kinematics of the HI in edge-on galaxies using a fit to the terminal-velocity channel maps of a HI data cube. The strategy c…

astro-ph.GA2016★ 5 cited

The Shape of Dark Matter Haloes II. The Galactus HI Modelling & Fitting Tool

S. P. C. Peters, P. C. van der Kruit, R. J. Allen +1

We present a new HI modelling tool called \textsc{Galactus}. The program has been designed to perform automated fits of disc-galaxy models to observations. It includes a treatment…

astro-ph.GA2016★ 18 cited

The Shape of Dark Matter Haloes, V. Analysis of observations of edge-on galaxies

S. P. C. Peters, P. C. van der Kruit, R. J. Allen +1

In the previous papers in this series, we have measured the stellar and \hi content in a sample of edge-on galaxies. In the present paper, we perform a simultaneous rotation curve…

astro-ph.GA2013

The Shape of Dark Matter Haloes, I. HI Observations of Edge-on Galaxies

S. P. C. Peters, P. C. van der Kruit, R. J. Allen +1

We present neutral hydrogen observations for a sample of eight nearby, late-type, edge-on galaxies. All of the galaxies have been well resolved in the radial direction, while six h…

astro-ph.CO2012★ 8 cited

The Opacity of Spiral Galaxy Disks IX; Dust and Gas Surface Densities

B. W. Holwerda, R. J. Allen, W. J. G. de Blok +4

Our aim is to explore the relation between gas, atomic and molecular, and dust in spiral galaxies. Gas surface densities are from atomic hydrogen and CO line emission maps. To esti…