  Recent evidence of super-Chandrasekhar white dwarfs (WDs), from the
observations of over-luminous type Ia supernovae (SNeIa), has been a great
astrophysical discovery. However, no such massive WDs have so far been observed
directly as their luminosities are generally quite low. Hence it immediately
raises the question of whether there is any possibility of detecting them
directly. The search for super-Chandrasekhar WDs is very important as SNeIa are
used as standard candles in cosmology. In this article, we show that continuous
gravitational wave can allow us to detect such super-Chandrasekhar WDs
directly.
