Detection of a Disk Surrounding the Variably Accreting Young Star HBC722
  We present new ALMA 233 GHz continuum observations of the FU Orionis Object
HBC722. With these data we detect HBC722 at millimeter wavelengths for the
first time, use this detection to calculate a circumstellar disk mass of 0.024
solar masses, and discuss implications for the burst triggering mechanism.
