  The spectroscopic and photometric analysis of sample Am stars are carried out
to determine the stellar characteristics of each studied star. The CCD
photometric analysis of HD 98851 and HD 207561 show clear evidence of pulsation
variability of 1.55 hr and 5.8 min respectively. Similarly, a clear evidence of
the photometric variability is also found for an Am star HD 73045 which is
likely to be pulsating in nature with a period of about 36-min. We are also
found dissimilar behaviour of elemental abundances of various ions for HD
113878 and HD 118660. The basic stellar parameters (mass, luminosity, radius,
life time, distance, proper-motion etc.) are determined for each sample stars.
The tidal radius and boundaries of habitable zone of each star are also
computed to search the extra-terrestrial life. Asteroseismic mass scale test
shows greater stellar masses compare to the solar mass.
