Gibb, A.G. and Little, L.T. (1995) HH24-26 - Structure, Dynmics and Chemistry. Astrophysics and Space Science, 224 . pp. 467-468. ISSN 0004-640X .
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New J=1-0 HCO+ and J=2-1 (CO)-O-18 observations of HH24-26 reveal striking differences between these and previous maps of higher-J transitions of HCO+ and CS. The hlgh-J HCO+ and CS emission traces the densest portions of the cloud, while (CO)-O-18 traces the more tenuous envelope. This is also evident in the velocity structure. HCO+ and (CO)-O-18 appear to be depleted from the gas phase by amounts which vary with position.
|Uncontrolled keywords:||MOLECULAR CLOUDS; HH24-26; ABUNDANCES; STRUCTURE|
|Subjects:||Q Science > QB Astronomy|
|Divisions:||Faculties > Science Technology and Medical Studies > School of Physical Sciences > Centre for Astrophysics and Planetary Sciences|
|Depositing User:||P. Ogbuji|
|Date Deposited:||01 Jun 2009 11:11|
|Last Modified:||08 May 2012 10:45|
|Resource URI:||http://kar.kent.ac.uk/id/eprint/19552 (The current URI for this page, for reference purposes)|
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