Astronomy and Astrophysics – Astrophysics – Solar and Stellar Astrophysics
Scientific paper
2009-02-03
Astronomy and Astrophysics
Astrophysics
Solar and Stellar Astrophysics
Accepted for publication in ApJL (2009 Feb 3)
Scientific paper
10.1088/0004-637X/694/1/L36
We present the results of a submillimeter interferometric survey of circumstellar disks in the Trapezium Cluster of Orion. We observed the 880 micron continuum emission from 55 disks using the Submillimeter Array, and detected 28 disks above 3sigma significance with fluxes between 6-70 mJy and rms noise between 0.7-5.3 mJy. Dust masses and upper limits are derived from the submillimeter excess above free-free emission extrapolated from longer wavelength observations. Above our completeness limit of 0.0084 solar masses, the disk mass distribution is similar to that of Class II disks in Taurus-Auriga and rho Ophiuchus but is truncated at 0.04 solar masses. We show that the disk mass and radius distributions are consistent with the formation of the Trapezium Cluster disks ~1 Myr ago and subsequent photoevaporation by the ultraviolet radiation field from Theta-1 Ori C. The fraction of disks which contain a minimum mass solar nebula within 60 AU radius is estimated to be 11-13% in both Taurus and the Trapezium Cluster, which suggests the potential for forming Solar Systems is not compromised in this massive star forming region.
Mann Rita K.
Williams Jonathan P.
No associations
LandOfFree
The Circumstellar Disk Mass Distribution in the Orion Trapezium Cluster does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Circumstellar Disk Mass Distribution in the Orion Trapezium Cluster, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Circumstellar Disk Mass Distribution in the Orion Trapezium Cluster will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-553024