J/ApJ/619/L95ivo://CDS.VizieR/J/ApJ/619/L95doi:10.26093/cds/vizier.16199095CDSXu C.K.Iglesias-Paramo J.Burgarella D.Rich R.M.Neff S.G.,Lauger S.Barlow T.A.Bianchi L.Byun Y.-I.Forster K.Friedman P.G.,Heckman T.M.Jelinsky P.N.Lee Y.-W.Madore B.F.Malina R.F.,Martin D.C.Milliard B.Morrissey P.Schiminovich D.Siegmund O.H.W.,Small T.Szalay A.S.Welsh B.Y.Wyder T.K.2018-09-29T16:12:51Z2014-06-05T15:38:24ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.fractive-galactic-nucleiinterstellar-mediumultraviolet-astronomyWe present the first Galaxy Evolution Explorer (GALEX) UV images of the well-known interacting group of galaxies, Stephan's Quintet (SQ). We detect widespread UV emission throughout the group. However, there is no consistent coincidence between UV structure and emission in the optical, H{alpha}, or HI. Excluding the foreground galaxy NGC 7320 (Sd), most of the UV emission is found in regions associated with the two spiral members of the group, NGC 7319 and NGC 7318b, and the intragroup medium starburst SQ-A. The extinction-corrected UV data are analyzed to investigate the overall star formation activity in SQ.2005ApJ...619L..95Xhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/619/L95CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/619/L95https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/619/L95http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/619/L95https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/619/L95https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/619/L95http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/619/L95GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapUVdefaultJ/ApJ/619/L95/table1Star formation properties in HCG 92 regionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName of the regionmeta.idcharf_Name[*] contribution of AGN subtracted (1)meta.codecharRegRegion number in FUV (see Fig.2a)meta.id;meta.maincharFUVFUV magnitude (1530{AA}), corrected for Galactic extinction (2)magphot.mag;em.UV.100-200nmfloate_FUVError in FUV (2)magstat.errorfloatlogLlog(L_FUV_), FUV luminosity (2) (3)log(solLum)phys.luminosity;em.UVfloate_logLError in logL (2)log(solLum)stat.errorfloatSFR? Star formation rate from L_FUV_ (2) (3)solMass/yrphys.SFRfloatnullablee_SFR? Error in SFR (2)solMass/yrstat.error;phys.SFRfloatnullableF-NFUV-NUV color index (NUV: 2310{AA}), corrected for Galactic extinction (2)magphot.color;em.UVfloate_F-NError in F-N (2)magstat.errorfloatlogtUV? log(stellar age) derived from extinction corrected FUV-NUV color index (3)log(yr)arith.zpfloatnullablee_logtUV? Error in logtUVlog(yr)stat.errorfloatnullableB-V? B-V color index, corrected for Galactic extinctionmagphot.color;em.opt.B;em.opt.Vfloatnullablee_B-V? Error in B-Vmagstat.error;phot.color;em.opt.BfloatnullablelogtBV? log(stellar age) derived from extinction corrected B-V color index (3)log(yr)arith.zpfloatnullablee_logtBV? Error in logtBVlog(yr)stat.errorfloatnullableAFUV? Internal extinction in the FUV band (3)magphys.absorption;em.UV.100-200nmfloatnullablee_AFUV? Error in AFUVmagstat.errorfloatnullable