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: email@example.com
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
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.