We have analysed the morphology, kinematics, colors and chemical composition of the ionized gas of the different objects belonging to the interacting compact group HCG 31 in order to get a global view of the origin and evolution of the dwarf galaxies present in it.
|Number of pages||2|
|Journal||Proceedings of the International Astronomical Union|
|Publication status||Published - 2004|
|Event||217th Symposium of the International-Astronomical-Union on Recycling Intergalactic and Interstellar Matter held at the 25th IAU General Assembly - Sydney, Australia|
Duration: 6 Aug 2002 → 10 Aug 2002