When galaxies interact the debris can coalesce to form new Tidal Dwarf
Galaxies (TDGs for short). This may be an important mechanism for the
formation of dwarf galaxies in the early universe. We have a Spitzer
program to observe a sample of Tidal Dwarf Galaxies. For details of
our research please read the following pages.
The first system we looked at is
NGC 5291
which is known for its tidal dwarf galaxy nursery.
This is our Spitzer IRAC image. Copyright Sarah Higdon/NASA.