Methyl Cyanide Observations Toward Massive Protostars
  We report the results of a survey in the CH3CN J= 12-11 transition toward a
sample of massive proto-stellar candidates. The observations were carried out
with the 10 m Submillimeter telescope on Mount Graham, AZ. We detected this
molecular line in 9 out of 21 observed sources. In six cases this is the first
detection of this transition. We also obtained full beam sampled cross-scans
for five sources which show that the lower K-components can be extended on the
arcminute angular scale. The higher K-components however are always found to be
compact with respect to our 36" beam. A Boltzmann population diagram analysis
of the central spectra indicates CH3CN column densities of about 10^14 cm^(-2),
and rotational temperatures above 50 K, which confirms these sources as hot
molecular cores. Independent fits to line velocity and width for the individual
K-components resulted in the detection of an increasing blue shift with
increasing line excitation for four sources. Comparison with mid-infrared
images from the SPITZER GLIMPSE/IRAC archive for six sources show that the
CH3CN emission is generally coincident with a bright mid-IR source. Our data
clearly show that the CH3CN J= 12-11 transition is a good probe of the hot
molecular gas near massive protostars, and provide the basis for future
interferometric studies.
