Anita L. Cochran, Edwin S. Barker, Candace L. Gray
We report on the results of a spectroscopic survey of 130 comets that was
conducted at McDonald observatory from 1980 through 2008. Some of the comets
were observed on only one night, while others were observed repeatedly. For 20
of these comets, no molecules were detected. For the remaining 110 comets, some
emission from CN, OH, NH, C$_{3}$, C$_{2}$, CH, and NH$_{2}$ molecules were
observed on at least one occasion. We converted the observed molecular column
densities to production rates using a Haser (1957) model. We defined a
restricted data set of comets that had at least 3 nights of observations. The
restricted data set consists of 59 comets. We used ratios of production rates
to study the trends in the data. We find two classes of comets: typical and
carbon-chain depleted comets. Using a very strict definition of depleted
comets, requiring C$_{2}$ \underline{and} C$_{3}$ to both be depleted, we find
9% of our restricted data set comets to be depleted. Using a more relaxed
definition that requires only C$_{2}$ to be below a threshold (similar to other
researchers), we find 25% of the comets are depleted. Two-thirds of the
depleted comets are Jupiter Family comets, while one-third are Long Period
comets. 37% of the Jupiter Family comets are depleted, while 18.5% of the Long
Period comets are depleted. We compare our results with other studies and find
good agreement.
View original:
http://arxiv.org/abs/1112.4770
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