protostellar IRAS sources made with high spatial resolution of 2.8-8.8 arcsec using the
Nobeyama millimeter array (NMA). Spatially extended CS emission is detected around all
the embedded sources and the two T Tauri stars DG Tau and HL Tau, while four T Tauri
stars and one embedded source L1551-IRS5 have detectable 98 GHz continuum emission
from unresolved circumstellar disks of 0.1 solar mass. It is inferred from the tendency of …