White, Glenn J. and Phillips, J. P.
Due to copyright restrictions, this file is not available for public download
|Google Scholar:||Look up in Google Scholar|
We have measured the 31,3-20,2 transition of SO2 in W49, W51, OriA and Sgr B2, and found SO2 emission upper limits in a further seven sources. The total number of SO2 molecules in individual clouds is found to range from ~2×1051 to ~1053, implying a relative abundance X(SO2) ~ 10-6 in OriA, and lower limits varying from X(SO2) ~ 10-9 to ~10-8 in the remaining sources. These results are briefly discussed within the context of current models of interstellar cloud chemistry.
|Item Type:||Journal Article|
|Copyright Holders:||1983 Royal Astronomical Society|
|Keywords:||interstellar chemistry; molecular clouds; sulfur dioxides; abundance; emission spectra; line spectra; molecular spectra|
|Academic Unit/Department:||Science > Physical Sciences|
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||07 Jun 2012 09:49|
|Last Modified:||17 Jul 2013 08:49|
|Share this page:|