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The Orion Nebula in the Far-Infrared: High-J CO and fine-structure lines mapped by FIFI-LS/SOFIA

Published online by Cambridge University Press:  31 March 2017

Randolf Klein ,
Leslie W. Looney ,
Erin Cox ,
Christian Fischer ,
Christof Iserlohe  and
Alfred Krabbe
Randolf Klein
Affiliation:
SOFIA-USRA, NASA Ames Research Center, MS 232-12, PO box 1, Moffet Field, CA 94035 email: [email protected]
Leslie W. Looney
Affiliation:
University of Illinois, Dept. of Astronomy, MC-221, 1002 W. Green St., Urbana, IL 61801
Erin Cox
Affiliation:
University of Illinois, Dept. of Astronomy, MC-221, 1002 W. Green St., Urbana, IL 61801
Christian Fischer
Affiliation:
Deutsches SOFIA Institut, Pfaffenwaldring 29, D-70569 Stuttgart
Christof Iserlohe
Affiliation:
Deutsches SOFIA Institut, Pfaffenwaldring 29, D-70569 Stuttgart
Alfred Krabbe
Affiliation:
Deutsches SOFIA Institut, Pfaffenwaldring 29, D-70569 Stuttgart
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Abstract

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The Orion Nebula is the closest massive star forming region allowing us to study the physical conditions in such a region with high spatial resolution. We used the far infrared integral-field spectrometer, FIFI-LS, on-board the airborne observatory SOFIA to study the atomic and molecular gas in the Orion Nebula at medium spectral resolution.

The large maps obtained with FIFI-LS cover the nebula from the BN/KL-object to the bar in several fine structure lines. They allow us to study the conditions of the photon-dominated region and the interface to the molecular cloud with unprecedented detail.

Another investigation targeted the molecular gas in the BN/KL region of the Orion Nebula, which is stirred up by a violent explosion about 500 years ago. The explosion drives a wide angled molecular outflow. We present maps of several high-J CO observations, allowing us to analyze the heated molecular gas.

Keywords

stars: formationinfrared: ISMISM: Orion Nebula
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S316: Formation, evolution, and survival of massive star clusters , August 2015 , pp. 153 - 154
Copyright
Copyright © International Astronomical Union 2017 

References

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