EAS Publications Series
Volume 31, 2008Far-Infrared Workshop 2007
|Page(s)||23 - 26|
|Published online||04 October 2008|
C. Kramer, S. Aalto and R. Simon (eds)
EAS Publications Series, 31 (2008) 23-26
Warm and dense gas and dust in Carina
KOSMA, I. Physikalisches Institut,
Universität zu Köln, Zülpicher Straße 77, 50937 Köln,
Corresponding author: firstname.lastname@example.org
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.
© EAS, EDP Sciences, 2008
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