A Submillimeter Array Survey of Protoplanetary Disks in the Orion Nebula Cluster
Rita K. Mann, Jonathan P. Williams

TL;DR
This survey of protoplanetary disks in the Orion Nebula using the Submillimeter Array reveals disk mass distributions, effects of proximity to massive stars, evidence of grain growth, and suggests potential for planet formation despite environmental erosion.
Contribution
First comprehensive submillimeter survey of Orion disks showing environmental impact on disk mass and evidence of grain growth, informing planet formation potential in massive star-forming regions.
Findings
Disks within 0.3 pc of theta^1 Ori C are truncated in mass.
Disk masses beyond 0.3 pc are similar to low-mass star forming regions.
Approximately 18% of disks have masses suitable for planet formation.
Abstract
We present the full results of our 3-year long Submillimeter Array survey of protoplanetary disks in the Orion Nebula Cluster. We imaged 23 fields at 880 microns and 2 fields at 1330 microns, covering an area of ~6.5 arcmin^2 and containing 67 disks. We detected 42 disks with fluxes between 6-135 mJy and at rms noise levels between 0.6 to 5.3 mJy/beam. Thermal dust emission above any free-free component was measured in 40 of the 42 detections, and the inferred disk masses range from 0.003-0.07 Msolar. We find that disks located within 0.3 pc of theta^1 Ori C have a truncated mass distribution, while disks located beyond 0.3 pc have masses more comparable to those found in low-mass star forming regions. The disk mass distribution in Orion has a distance dependence, with a derived relationship max(M_(disk)) = 0.046Msolar(d/0.3pc)^0.33 for the maximum disk masses. We found evidence of…
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