@misc{10481/28407,
year = {2006},
url = {http://hdl.handle.net/10481/28407},
abstract = {Star formation in interacting systems may take place in various locations, from the dust--enshrouded core of Ultraluminous Infrared Galaxies to more unusual places such as the debris of colliding galaxies expelled into the intergalactic medium. Determining whether star-formation proceeds in the latter environment, far from the parent galaxies, in a similar way as in spiral disks has motivated the multi--wavelength study presented here. We collected VLA/HI, UV/GALEX, optical Halpha and MIR/Spitzer images of a few nearby interacting systems chosen for their prominent "intergalactic" star formation activity. Preliminary results on the spectacular collisional HI ring around NGC 5291 are presented.},
keywords = {Galaxies},
keywords = {Star formation},
keywords = {NGC 5291},
title = {Intergalactic star formation},
author = {Duc, P.-A. and Boquien, Mérédic and Braine, J. and Brinks, E. and Lisenfeld , Ute and Charmandaris, V.},
}