A Mid-IR Study of the L1641-N Region with ISOCAM

Details A Mid-IR Study of the L1641-N Region with ISOCAM A Mid-IR Study of the L1641-N Region with ISOCAM

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aas...198.4806a&link_type=abstract

American Astronomical Society, 198th AAS Meeting, #48.06; Bulletin of the American Astronomical Society, Vol. 33, p.851

Astronomy and Astrophysics

Astronomy

Scientific paper

The L1641-N outflow region (part of the sourthern Orion A cloud) was imaged with ISOCAM in both broad-band (LW2, 7um and LW3, 15um) and narrow-band CVF (5-17 um) by the Infrared Space Observatory (ISO) array CAMera (ISOCAM). We present a new analysis this data set based on customized reduction schemes developed at IPAC as part of the IPAC ISO star-formation "templates" project. The purpose of the IPAC templates is to provide the best-possible, customized reduction of ISO data on all star-forming regions. In this contribution we discuss ISOCAM reduction methods and present some preliminary results.

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