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12-μm fine-structure emission line and continuum images of G333.6-0.2

Abstract:
We present high spatial resolution (∼0.8 arcsec) diffraction-limited 12.8-μm Ne II fine-structure emission line and 12.5-μm continuum images of the bright southern compact H II region G333.6-0.2, taken with the mid-infrared imaging polarimeter NIMPOL. The two images show remarkably similar, compact, yet asymmetric, flux distributions. The [Ne II] image shows a complex structure near the ionizing source(s) which we interpret in terms of the ionization structure of the H II region. It is found that G333.6-0.2 is more likely to be excited by a cluster of O and B stars than by a single star.

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Role:
Author


Journal:
Monthly Notices of the Royal Astronomical Society More from this journal
Volume:
296
Issue:
2
Pages:
225-230
Publication date:
1998-05-11
ISSN:
0035-8711


Language:
English
Keywords:
Pubs id:
pubs:345202
UUID:
uuid:1c15c20f-281f-4d10-b9c2-08dc8aecc61b
Local pid:
pubs:345202
Source identifiers:
345202
Deposit date:
2012-12-19
ARK identifier:

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