  The spectroscopic observations of two novae namely V1065 CEN and V1280 SCO
were made by 45 cm Cassegrain telescope in high resolution
($\lambda/\delta\lambda$=22000) at H$\alpha$ (6563 \r{A}) region. V1065 CEN is
He/N-type spectra which characterize a broad (Gaussian FWHM 49 \r{A}), saddle
shaped and asymmetric H$\alpha$ emission line without prominent P-Cyg
absorption component. Completely different H$\alpha$ profile of V1280 SCO shows
prominent P-Cyg absorption and narrow emission line (Gaussian FWHM 26 \r{A})
which can be classified as Fe II type nova. The expansion velocities of these
two systems measured from the minima of the P-Cyg profiles are close to 2300
km/s for V1065 CEN, and 716 km/s for V1280 SCO. Based on the photometric
analysis, the Nova V1065 CEN can be classified as fast (11$<$t${_2}$$<$25)
nova. The derived absolute magnitudes at maximum for nova V1065 CEN to be
M$_{o,V}$ = -7.58$\pm$0.18 and M$_{o,B}$= -7.75$\pm$0.25 correspond to a
distance 8.51$\pm$0.33 kpc. The parameters t$_{2V}$=12 days and t$_{3V}$=14
days of nova V1280 SCO determine that the nova is in between very fast and fast
nova. The mean absolute magnitude at maximum is calculated to be
M$_{o,V}$=-8.7$\pm$0.1 and the estimated distance to the nova V1280 SCO is
3.2$\pm$0.2 kpc.
