Afficher la notice abrégée

dc.contributor.authorNatale, G.
dc.contributor.authorTuffs, Richard J.
dc.contributor.authorXu, C. K.
dc.contributor.authorPopescu, Cristina C.
dc.contributor.authorFischera, J.
dc.contributor.authorLisenfeld , Ute 
dc.contributor.authorLu, N.
dc.contributor.authorAppleton, P. N.
dc.contributor.authorDopita, M.
dc.contributor.authorDuc, P.-A.
dc.contributor.authorGao, Y.
dc.contributor.authorReach, W.
dc.contributor.authorSulentic, J.
dc.contributor.authorYun, M. S.
dc.date.accessioned2013-10-07T12:23:56Z
dc.date.available2013-10-07T12:23:56Z
dc.date.issued2012
dc.identifier.citationNatale, G.; et al. The star formation efficiency in Stephan's Quintet intragroup regions. In: Wei-Hsin Sun (ed). Galaxi mergers in an evolving universe, 2011. ASP Conference Series. [http://hdl.handle.net/10481/28320]es_ES
dc.identifier.issn1050-3390
dc.identifier.otherarXiv:1203.3436v1
dc.identifier.urihttp://hdl.handle.net/10481/28320
dc.descriptionConference proceedings "Galaxy Mergers in an evolving Universe", 23-28 October 2011, Hualien, Taiwan.es_ES
dc.description.abstractWe investigated the star formation efficiency for all the dust emitting sources in Stephan's Quintet (SQ). We inferred star formation rates using Spitzer MIR/FIR and GALEX FUV data and combined them with gas column density measurements by various authors, in order to position each source in a Kennicutt-Schmidt diagram. Our results show that the bright IGM star formation regions in SQ present star formation efficiencies consistent with those observed within local galaxies. On the other hand, star formation in the intergalactic shock region seems to be rather inhibited.es_ES
dc.language.isoenges_ES
dc.publisherAstronomical Society of the Pacifices_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.subjectAstrophysics es_ES
dc.subjectStephan's Quintetes_ES
dc.subjectGalaxies es_ES
dc.subjectStar formationes_ES
dc.titleThe star formation efficiency in Stephan's Quintet intragroup regionses_ES
dc.typepreprintes_ES
dc.rights.accessRightsopen accesses_ES


Fichier(s) constituant ce document

[PDF]

Ce document figure dans la(les) collection(s) suivante(s)

Afficher la notice abrégée

Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License
Excepté là où spécifié autrement, la license de ce document est décrite en tant que Creative Commons Attribution-NonCommercial-NoDerivs 3.0 License