Classification of stellar spectra by human experts, in the past, has b
een subjective, leading to many nonunique databases. However, with the
availability of large spectral databases, automated classification sc
hemes offer an alternative to visual classification. Here, we present
two schemes for automated classification of stellar spectra, namely, c
hi2-minimization and Artificial Neural Network. These techniques have
been applied to classify a complete set of 158 test spectra into 55 sp
ectral types of a reference library. Using these methods, we have succ
essfully classified the test library on the basis of reference library
to an accuracy of two spectral subclasses. Such automated schemes wou
ld in the future provide fast, uniform, and almost on-line classificat
ion of stellar spectra.