The nature of supernovae 2010O and 2010P in Arp 299-II. Radio emission

Simple item page
dc.contributor.authorRomero Canizales, C.
dc.contributor.authorHerrero Illana, R.
dc.contributor.authorPerez Torres, M. A.
dc.contributor.authorAlberdi, A.
dc.contributor.authorKankare, E.
dc.contributor.authorBauer, F. E.
dc.contributor.authorRyder, S. D.
dc.contributor.authorMattila, S.
dc.contributor.authorConway, J. E.
dc.contributor.authorBeswick, R. J.
dc.contributor.authorMuxlow, T. W. B.
dc.date.accessioned2024-01-10T13:43:52Z
dc.date.available2024-01-10T13:43:52Z
dc.date.issued2014
dc.description.abstractWe report radio observations of two stripped-envelope supernovae (SNe), 2010O and 2010P, which exploded within a few days of each other in the luminous infrared galaxy Arp 299. Whilst SN 2010O remains undetected at radio frequencies, SN 2010P was detected (with an astrometric accuracy better than 1 milli arcsec in position) in its optically thin phase in epochs ranging from similar to 1 to similar to 3 yr after its explosion date, indicating a very slow radio evolution and a strong interaction of the SN ejecta with the circumstellar medium. Our late-time radio observations towards SN 2010P probe the dense circumstellar envelope of this SN, and imply M [M-circle dot yr(-1)]/upsilon(wind) [10 km s(-1)] = (3.0 - 5.1) x 10(-5), with a 5 GHz peak luminosity of similar to 1.2 x 10(27) erg s(- 1) Hz(- 1) on day similar to 464 after explosion. This is consistent with a Type IIb classification for SN 2010P, making it the most distant and most slowly evolving Type IIb radio SN detected to date.
dc.description.funderEuropean Commission
dc.description.funderAcademy of Finland
dc.description.funderBasal-CATA
dc.description.funderCONICYT-Chile
dc.description.funderALMA-CONICYT FUND Project
dc.description.funderIniciativa Cientifica Milenio grant
dc.description.funderSpanish MINECO
dc.description.funderFEDER funds
dc.description.funderJenny and Antti Wihuri Foundation
dc.description.funderScience and Technology Facilities Council
dc.format.extent13 páginas
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/stu430
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stu430
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/78778
dc.identifier.wosidWOS:000334742200010
dc.information.autorucAstrofísica;Bauer F;S/I;1007961
dc.information.autorucAstrofísica;Romero-Canizales C;S/I;1012111
dc.issue.numero2
dc.language.isoen
dc.nota.accesoSin adjunto
dc.pagina.final1079
dc.pagina.inicio1067
dc.publisherOXFORD UNIV PRESS
dc.revistaMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.rightsregistro bibliográfico
dc.subjectsupernovae: general
dc.subjectsupernovae: individual: SN 2010O
dc.subjectsupernovae: individual: SN 2010P
dc.subjectgalaxies: individual: Arp 299
dc.subjectgalaxies: starburst
dc.subjectradio continuum: galaxies
dc.subjectLUMINOUS INFRARED GALAXY
dc.subjectX-RAY-EMISSION
dc.subjectLIGHT-CURVES
dc.subjectSN 2011DH
dc.subjectMODULATIONS
dc.subjectPROGENITORS
dc.subjectEVOLUTION
dc.subjectEXPLOSION
dc.subjectDISCOVERY
dc.subjectREVEAL
dc.subject.ods07 Affordable and Clean Energy
dc.subject.odspa07 Energía asequible y no contaminante
dc.titleThe nature of supernovae 2010O and 2010P in Arp 299-II. Radio emission
dc.typeartículo
dc.volumen440
sipa.codpersvinculados1007961
sipa.codpersvinculados1012111
sipa.indexWOS
sipa.indexScopus
sipa.trazabilidadCarga SIPA;09-01-2024
Files
Collections
Artículos de revistas