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Warm and dense gas and dust in Carina

Published online by Cambridge University Press:  04 October 2008

C. Kramer ,
S. Aalto ,
R. Simon  and
C. Kramer
C. Kramer*
Affiliation:
KOSMA, I. Physikalisches Institut, Universität zu Köln, Zülpicher Straße 77, 50937 Köln, Germany
*
[email protected]
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Abstract

The NANTEN2-4 m submillimeter telescope was used to map the [C i] 3P1-3PP0, 3P2-3P1 and CO 4–3, 7–6 lines in two 4'×4' regions of Carina where molecular material interfaces with radiation from the massive star clusters. These data were combined with 13CO SEST spectra, HIRES/IRAS maps at 60 µm, 100 µmm, maps of 8 µmm IRAC/Spitzer, and of MSX emission. We use PDR models to interpret the observed far-infrared and submillimeter emission, assuming that all observed emission stems from an ensemble of spherically symmetric PDR clumps.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 31: Far-Infrared Workshop 2007 , 2008 , pp. 23 - 26
Copyright
© EAS, EDP Sciences, 2008

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References

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