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Mid-IR Imaging of Orion BN/KL: Modeling of Physical Conditions and Energy Balance

Published online by Cambridge University Press:  12 September 2016

Daniel Gezari
Affiliation:
Code 667, NASA/GSFC, Greenbelt, MD 20771USA; email: Daniel.Y.Gezari@nasa.gov
Frank Varosi
Affiliation:
Univ. of Florida-Gainesville, USA
Eli Dwek
Affiliation:
Code 667, NASA/GSFC, Greenbelt, MD 20771USA; email: Daniel.Y.Gezari@nasa.gov
William Danchi
Affiliation:
Code 667, NASA/GSFC, Greenbelt, MD 20771USA; email: Daniel.Y.Gezari@nasa.gov
Jonathan Tan
Affiliation:
Univ. of Florida-Gainesville, USA
Shin-ichiro Okumura
Affiliation:
Okayama Astro. Observatory, Japan
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We have modeled two mid-infrared imaging photometry data sets to determine the spatial distribution of physical conditions in the BN/KL infrared complex. We observed the BN/KL region using the 10-m Keck I telescope and the LWS in the direct imaging mode, over a 13” × 19” field (Figure 1, left). We also modeled images obtained with COMICS (Kataza et al. 2000) at the 8.2-m SUBARU telescope, over a total field of view is 31” × 41” (Figure 1, right), in a total of nine bands: 7.8, 8.8, 9.7, 10.5, 11.7, 12.4, 18.5, 20.8 and 24.8 μm with ~1 μm bandwidth interference filters.

Type
Poster Papers
Copyright
Copyright © International Astronomical Union 2016 

References

Kataza, H., Okamoto, Y., Takubo, S., Onaka, T., Sako, S., Nakamura, K., Miyata, T., Yamashita, T. 2000, Proc. SPIE, 4008, 1144.CrossRefGoogle Scholar
Okumura, S., Yamashita, T., Sako, S., Miyata, T., Honda, M., Kataza, H., Okamoto, Y. 2011 PASJ, 63 (4), 823834.CrossRefGoogle Scholar
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Varosi, F., 2015, private communication.Google Scholar