  In this work, we present the new catalog of carbon stars from the LAMOST DR2
catalog. In total, 894 carbon stars are identified from multiple line indices
measured from the stellar spectra. Combining the CN bands in the red end with
\ctwo\ and other lines, we are able to identify the carbon stars. Moreover, we
also classify the carbon stars into spectral sub-types of \ch, \CR, and \cn.
These sub-types approximately show distinct features in the multi-dimensional
line indices, implying that in the future we can use them to identify carbon
stars from larger spectroscopic datasets. Meanwhile, from the line indices
space, while the \cn\ stars are clearly separated from the others, we find no
clear separation between \CR\ and \ch\ sub-types. The \CR\ and \ch\ stars seem
to smoothly transition from one to another. This may hint that the \CR\ and
\ch\ stars may not be different in their origins but look different in their
spectra because of different metallicity. Due to the relatively low spectral
resolution and lower signal-to-noise ratio, the ratio of $^{12}$C/$^{13}$C is
not measured and thus the \cj\ stars are not identified.
