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Detection of H2O Emission from the Far-Infrared Source AFCRL(UOA)19

White, G.J., Little, L.T., Parker, Edward A., Nicholson, P.S., Macdonald, G.H., Bales, F. (1975) Detection of H2O Emission from the Far-Infrared Source AFCRL(UOA)19. Monthly Notices of the Royal Astronomical Society, 170 (1). pp. 37-38. ISSN 0035-8711. E-ISSN 1365-2966. (doi:10.1093/mnras/170.1.37P) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:43188)

The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided.
Official URL:
http://dx.doi.org/10.1093/mnras/170.1.37P

Abstract

We have detected 22.2 GHz radiation from interstellar water vapour in the far infrared source AFCRL (UOA) 19. The H2O source does not appear to be dynamically associated with the CO, HCN and CS clouds already detected in AFCRL (UOA) 19.

Item Type: Article
DOI/Identification number: 10.1093/mnras/170.1.37P
Subjects: Q Science > QB Astronomy
Divisions: Divisions > Division of Computing, Engineering and Mathematical Sciences > School of Engineering and Digital Arts
Depositing User: Ted Parker
Date Deposited: 06 Oct 2014 09:36 UTC
Last Modified: 16 Nov 2021 10:17 UTC
Resource URI: https://kar.kent.ac.uk/id/eprint/43188 (The current URI for this page, for reference purposes)

University of Kent Author Information

Parker, Edward A..

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Macdonald, G.H..

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