Spitzer IRAC Detection of Protostellar Outflows

Details Spitzer IRAC Detection of Protostellar Outflows Spitzer IRAC Detection of Protostellar Outflows

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21341310y&link_type=abstract

American Astronomical Society, AAS Meeting #213, #413.10; Bulletin of the American Astronomical Society, Vol. 41, p.221

Astronomy and Astrophysics

Astronomy

Scientific paper

We will discuss a method for detecting shocked H2 emission in IRAC band images and distinguishing H2 knots from stellar sources. Using this method we will present Spitzer IRAC imaging of a recently discovered parsec scale protostellar outflow. This outflow was detected in all four IRAC bands. The proposed source of the outflow is an embedded Class 0 object detected in the MIPS images.
This work is based in part on archival data obtained with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. Support for this work was provided by an award issued by JPL/Caltech and also a NASA LTSA Grant NNG05GD66G

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