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Intergalactic star formation

dc.contributor.authorDuc, P.-A.
dc.contributor.authorBoquien, Mérédic
dc.contributor.authorBraine, J.
dc.contributor.authorBrinks, E.
dc.contributor.authorLisenfeld , Ute 
dc.contributor.authorCharmandaris, V.
dc.date.accessioned2013-10-10T10:44:02Z
dc.date.available2013-10-10T10:44:02Z
dc.date.issued2006
dc.identifier.citationDuc, 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.otherarXiv:astro-ph/0610392v1
dc.identifier.urihttp://hdl.handle.net/10481/28407
dc.description.abstractStar 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.isoenges_ES
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivs 3.0 Licensees_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es_ES
dc.subjectGalaxies es_ES
dc.subjectStar formationes_ES
dc.subjectNGC 5291es_ES
dc.titleIntergalactic star formationes_ES
dc.typeconference outputes_ES
dc.rights.accessRightsopen accesses_ES


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