NGC 2146 is a barred spiral galaxy in the
constellation of Camelopardalis. This peculiar galaxy with large
arms and a large nuclear disk exhibits a warped tidal shape
structure that is believed to be the result of a close encounter
or merger with a companion galaxy approximately 800,000 years
ago though no companion is visible today. This event is believed
to be the cause for high starburst activity within the galaxy
center as evident by the bright core. Starburst activity is when
stars form at a much higher rate than those in normal galaxies.
