The Open UniversitySkip to content
 

CO J= 3→2 and J= 2→1 observations of the Kleinmann-Low nebula

Phillips, J. P.; White, Glenn J. and Watt, Graeme D. (1982). CO J= 3→2 and J= 2→1 observations of the Kleinmann-Low nebula. Monthly Notices of the Royal Astronomical Society, 199 pp. 1033–1044.

Full text available as:
Full text not publicly available
Due to copyright restrictions, this file is not available for public download
URL: http://articles.adsabs.harvard.edu//full/seri/MNRA...
Google Scholar: Look up in Google Scholar

Abstract

An area of sky centred on the Kleinmann-Low nebula has been mapped in the J = 3 → 2 and J = 2 → 1 lines of CO. There appears evidence for asymmetry of the "pedestal" emission to the west of the source centre, probably indicative of an irregular mass distribution. This is discussed in the context of two models of the high-velocity gas, namely high-velocity nonisotropic outflow, and rotation within a compact cloud. Although the present observations do not enable us to discriminate between these, the presence of optically thin CO emission in this source is shown to lead to severe structural constraints on any rotational model. The suggestion that such a model may also lead to an over-abundance of high-velocity stars is not verified by the present analyses.

Item Type: Journal Article
Copyright Holders: 1982 Royal Astronomical Society
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
Item ID: 33795
Depositing User: Glenn White
Date Deposited: 06 Jun 2012 13:54
Last Modified: 06 Jun 2012 14:24
URI: http://oro.open.ac.uk/id/eprint/33795
Share this page:

Actions (login may be required)

View Item
Report issue / request change

Policies | Disclaimer

© The Open University   + 44 (0)870 333 4340   general-enquiries@open.ac.uk