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The gas-to-dust mass ratio of Centaurus A as seen...
Journal article

The gas-to-dust mass ratio of Centaurus A as seen by Herschel*

Abstract

We present photometry of the nearby galaxy NGC 5128 (Centaurus A) observed with the Photodetector Array Camera and Spectrometer (PACS) and Spectral and Photometric Imaging Receiver (SPIRE) instruments on board the Herschel Space Observatory, at 70, 160, 250, 350 and 500 μm, as well as new CO J= 3–2 observations taken with the HARP-B instrument on the James Clerk Maxwell Telescope (JCMT). Using a single-component modified blackbody, we model the …

Authors

Parkin TJ; Wilson CD; Foyle K; Baes M; Bendo GJ; Boselli A; Boquien M; Cooray A; Cormier D; Davies JI

Journal

Monthly Notices of the Royal Astronomical Society, Vol. 422, No. 3, pp. 2291–2301

Publisher

Oxford University Press (OUP)

Publication Date

May 21, 2012

DOI

10.1111/j.1365-2966.2012.20778.x

ISSN

0035-8711