Abstract
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.
Original language | English |
---|---|
Pages (from-to) | 568-569 |
Number of pages | 2 |
Journal | Proceedings of the International Astronomical Union |
Volume | 217 |
DOIs | |
Publication status | Published - 2004 |
Externally published | Yes |
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 |