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Molecular line mapping of the giant molecular cloud associated with RCW 106 – III. Multimolecular line mapping.

Authors :
Lo, N.
Cunningham, M. R.
Jones, P. A.
Bains, I.
Burton, M. G.
Wong, T.
Muller, E.
Kramer, C.
Ossenkopf, V.
Henkel, C.
Deragopian, G.
Donnelly, S.
Ladd, E. F.
Source :
Monthly Notices of the Royal Astronomical Society; May2009, Vol. 395 Issue 2, p1021-1042, 22p, 11 Charts, 15 Graphs, 6 Maps
Publication Year :
2009

Abstract

We present multimolecular line maps obtained with the Mopra telescope towards the southern giant molecular cloud (GMC) complex G333, associated with the H ii region RCW 106. We have characterized the GMC by decomposing the 3D data cubes withgaussclumps, and investigated spatial correlations among different molecules with principal component analysis (PCA). We find no correlation between clump size and linewidth, but a strong correlation between emission luminosity and linewidth. PCA classifies molecules into high- and low-density tracers, and reveals that HCO<superscript>+</superscript> and N<subscript>2</subscript>H<superscript>+</superscript> are anticorrelated. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
00358711
Volume :
395
Issue :
2
Database :
Complementary Index
Journal :
Monthly Notices of the Royal Astronomical Society
Publication Type :
Academic Journal
Accession number :
38218796
Full Text :
https://doi.org/10.1111/j.1365-2966.2009.14594.x