SPITZERAND NEAR-INFRARED OBSERVATIONS OF A NEW BIPOLAR PROTOSTELLAR OUTFLOW IN THE ROSETTE MOLECULAR CLOUD
Autor: | Jason E. Ybarra, Zoltan Balog, Randy L. Phelps, Elizabeth A. Lada, Scott W. Fleming |
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Rok vydání: | 2010 |
Předmět: |
Physics
Infrared Astrophysics::High Energy Astrophysical Phenomena Molecular cloud Near-infrared spectroscopy FOS: Physical sciences Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics Rosette (botany) Astrophysics - Solar and Stellar Astrophysics Space and Planetary Science Coincident Astrophysics::Solar and Stellar Astrophysics Outflow Astrophysics::Earth and Planetary Astrophysics Absorption (electromagnetic radiation) Solar and Stellar Astrophysics (astro-ph.SR) Astrophysics::Galaxy Astrophysics |
Zdroj: | The Astrophysical Journal. 714:469-475 |
ISSN: | 1538-4357 0004-637X |
DOI: | 10.1088/0004-637x/714/1/469 |
Popis: | We present and discuss \emph{Spitzer} and near-infrared H$_{2}$ observations of a new bi-polar protostellar outflow in the Rosette Molecular Cloud. The outflow is seen in all four IRAC bands and partially as diffuse emission in the MIPS 24 $\mu$m band. An embedded MIPS 24 $\mu$m source bisects the outflow and appears to be the driving source. This source is coincident with a dark patch seen in absorption in the 8 $\mu$m IRAC image. \emph{Spitzer} IRAC color analysis of the shocked emission was performed from which thermal and column density maps of the outflow were constructed. Narrow-band near-infrared (NIR) images of the flow reveal H$_2$ emission features coincident with the high temperature regions of the outflow. This outflow has now been given the designation MHO 1321 due to the detection of NIR H$_2$ features. We use these data and maps to probe the physical conditions and structure of the flow. Comment: Accepted for publication in The Astrophysical Journal |
Databáze: | OpenAIRE |
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