The distribution of atomic gas and dust in nearby galaxies - II. Further matched-resolution Very Large Array H i and SCUBA 850-μm images

Thomas, H. C., Dunne, Loretta, Green, D. A., Clemens, M. S., Alexander, P. and Eales, Stephen Anthony ORCID: https://orcid.org/0000-0002-7394-426X 2004. The distribution of atomic gas and dust in nearby galaxies - II. Further matched-resolution Very Large Array H i and SCUBA 850-μm images. Monthly Notices of the Royal Astronomical Society 348 (4) , pp. 1197-1207. 10.1111/j.1365-2966.2004.07491.x

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Abstract

We present Very Large Array (VLA) C-array 21-cm H i images of galaxies from the SCUBA Local Universe Galaxy Survey which have been observed at 850 μm with the James Clerk Maxwell Telescope. Matched-resolution (∼ 25 arcsec) H i images of 17 galaxies are presented and compared with 850-μm images. H i or 850-μm images of an additional six galaxies which were detected at only one wavelength are presented. Additionally, lower resolution H i observations of nine galaxies are presented. The observations of these galaxies, along with results previously presented, do not show any obvious trends in the H i/dust or H2/dust mass ratios with morphological type.

Item Type:	Article
Date Type:	Publication
Status:	Published
Schools:	Physics and Astronomy
Subjects:	Q Science > QB Astronomy
Uncontrolled Keywords:	galaxies; abundances; ISM; structure; radio lines
Additional Information:	Pdf uploaded in accordance with publisher's policy at http://www.sherpa.ac.uk/romeo/issn/0035-8711/ (accessed 20/02/2014).
Publisher:	Royal Astronomical Society
ISSN:	0035-8711
Date of First Compliant Deposit:	30 March 2016
Last Modified:	04 May 2023 19:03
URI:	https://orca.cardiff.ac.uk/id/eprint/47003

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