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Intergalactic star formation
dc.contributor.author | Duc, P.-A. | |
dc.contributor.author | Boquien, Mérédic | |
dc.contributor.author | Braine, J. | |
dc.contributor.author | Brinks, E. | |
dc.contributor.author | Lisenfeld , Ute | |
dc.contributor.author | Charmandaris, V. | |
dc.date.accessioned | 2013-10-10T10:44:02Z | |
dc.date.available | 2013-10-10T10:44:02Z | |
dc.date.issued | 2006 | |
dc.identifier.citation | Duc, P.-A.; et al. Intergalactic star formation. In: Studying galaxy evolution wiht Spitzer and Herschel. Crete (Greece) may 28- june 2 (2006). [http://hdl.handle.net/10481/28407] | es_ES |
dc.identifier.other | arXiv:astro-ph/0610392v1 | |
dc.identifier.uri | http://hdl.handle.net/10481/28407 | |
dc.description.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. | es_ES |
dc.language.iso | eng | es_ES |
dc.rights | Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License | es_ES |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/3.0/ | es_ES |
dc.subject | Galaxies | es_ES |
dc.subject | Star formation | es_ES |
dc.subject | NGC 5291 | es_ES |
dc.title | Intergalactic star formation | es_ES |
dc.type | info:eu-repo/semantics/conferenceObject | es_ES |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | es_ES |