HH24-26 - Structure, Dynmics and Chemistry

Gibb, A.G., Little, L.T. (1995) HH24-26 - Structure, Dynmics and Chemistry. Astrophysics and Space Science, 224 . pp. 467-468. ISSN 0004-640X. (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:19552)

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.

Abstract

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.

Item Type:	Article
Uncontrolled keywords:	MOLECULAR CLOUDS; HH24-26; ABUNDANCES; STRUCTURE
Subjects:	Q Science > QB Astronomy
Divisions:	Divisions > Division of Natural Sciences > Physics and Astronomy
Depositing User:	P. Ogbuji
Date Deposited:	01 Jun 2009 11:11 UTC
Last Modified:	05 Nov 2024 09:56 UTC
Resource URI:	https://kar.kent.ac.uk/id/eprint/19552 (The current URI for this page, for reference purposes)

University of Kent Author Information

Little, L.T..

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