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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
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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.
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- 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
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2011
PASJ, 63
(4), 823–834.CrossRefGoogle Scholar
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