Kavli Affiliate: Feng Long| Summary: We have performed Submillimeter Array (SMA) observations of 198.0-407.5 GHz broadband spectra of 10 Class II protoplanetary disks in the Taurus-Auriga region. The 337 GHz flux densities ($F_rm 337 GHz$) of these objects are in the range of 8.2-34 mJy. The median and standard deviation of the 198-358 GHz spectral […]
Continue.. SMA 200-400 GHz Survey for 10 faint Class II Disks in the Taurus Molecular Cloud