A new mid - infrared map of the BN / KL region using the Keck telescope

We present a new mid-infrared (12.5 μm) map of the BN/KL high-mass star-forming complex in Orion using the LWS instrument at Keck I. Despite poor weather we achieved nearly diffraction-limited images (FWHM = 0.38) over a roughly 25×25 region centered on IRc2 down to a flux limit of ≈ 250 mJy. Many of the known infrared (IR) sources in the region break up into smaller sub-components. We have also detected 6 new mid-IR sources. Nearly all of the sources are resolved in our mosaic. The near-IR source “n” is slightly elongated in the mid-IR along a NW–SE axis and perfectly bisects the double-peaked radio source “L”. Source n has been identified as a candidate for powering the large IR luminosity of the BN/KL region (L = 10 L⊙). We postulate that the 12 μm emission arises in a circumstellar disk surrounding source n. The morphology of the mid-IR emission and the Orion “hot core” (as seen in NH3 emission), along with the location of water and OH masers, is very suggestive of a bipolar cavity centered on source n and aligned with the rotation axis of the hypothetical circumstellar disk. IRc2, once thought to be the dominant energy source for the BN/KL region, clearly breaks into 4 sub-sources in our mosaic, as seen previously at 3.8 – 5.0 μm. The anti-correlation of mid-IR emission and NH3 emission from the nearby hot core indicates that the IRc2 sources are roughly coincident (or behind) the dense hot core. The nature of IRc2 is not clear: neither self-luminous sources (embedded protostars) nor external heating by source I can be definitively ruled out. We also report the discovery of a new arc-like feature SW of the BN object, and some curious morphology surrounding near-IR source