CO Core Candidates in the Gemini Molecular Cloud
  We present observations of a 4 squared degree area toward the Gemini cloud
obtained using J = 1-0 transitions of $^{12}$CO, $^{13}$CO and C$^{18}$O. No
C$^{18}$O emission was detected. This region is composed of 36 core candidates
of $^{13}$CO. These core candidates have a characteristic diameter of 0.25 pc,
excitation temperatures of 7.9 K, line width of 0.54 km s$^{-1}$ and a mean
mass of 1.4 M$_{\sun}$. They are likely to be starless core candidates, or
transient structures, which probably disperse after $\sim$10$^6$ yr.
