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                          <header>
                              <identifier>oai:research.chalmers.se:199462</identifier>
                              <datestamp>2018-05-30T14:01:55Z</datestamp>
                              <setSpec>openaire</setSpec>
                          </header>
                          <metadata>
                              <oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
                                  <dc:title>The nature of supernovae 2010O and 2010P in Arp 299 - II. Radio emission</dc:title>
                                  <dc:identifier>https://research.chalmers.se/en/publication/199462</dc:identifier>
                                  <dc:date>2014</dc:date>
                                              <dc:creator>Romero-Cañizales, C.</dc:creator>
                                              <dc:creator>Herrero-Illana, R.</dc:creator>
                                              <dc:creator>Perez-Torres, Miguel Angel</dc:creator>
                                              <dc:creator>Alberdi, Antxon</dc:creator>
                                              <dc:creator>Kankare, E.</dc:creator>
                                              <dc:creator>Bauer, F. E.</dc:creator>
                                              <dc:creator>Ryder, S. D.</dc:creator>
                                              <dc:creator>Mattila, S.</dc:creator>
                                              <dc:creator>Conway, John</dc:creator>
                                              <dc:creator>Beswick, R. J.</dc:creator>
                                              <dc:creator>Muxlow, T .W. B.</dc:creator>
                                                  <dc:subject>Astronomy, Astrophysics and Cosmology</dc:subject>
                                              <dc:subject>1982</dc:subject>
                                              <dc:subject>V267</dc:subject>
                                              <dc:subject>ASTROPHYSICAL JOURNAL</dc:subject>
                                              <dc:subject>DISCOVERY</dc:subject>
                                              <dc:subject>radio continuum: galaxies</dc:subject>
                                              <dc:subject>LIGHT-CURVES</dc:subject>
                                              <dc:subject>EXPLOSION</dc:subject>
                                              <dc:subject>supernovae: general</dc:subject>
                                              <dc:subject>X-RAY-EMISSION</dc:subject>
                                              <dc:subject>LUMINOUS INFRARED GALAXY</dc:subject>
                                              <dc:subject>supernovae: individual: SN 2010O</dc:subject>
                                              <dc:subject>PROGENITORS</dc:subject>
                                              <dc:subject>REVEAL</dc:subject>
                                              <dc:subject>galaxies: starburst</dc:subject>
                                              <dc:subject>supernovae: individual: SN 2010P</dc:subject>
                                              <dc:subject>SN 2011DH</dc:subject>
                                              <dc:subject>MODULATIONS</dc:subject>
                                              <dc:subject>1983</dc:subject>
                                              <dc:subject>galaxies: individual: Arp 299</dc:subject>
                                              <dc:subject>P551</dc:subject>
                                              <dc:subject>EVALIER RA</dc:subject>
                                              <dc:subject>V259</dc:subject>
                                              <dc:subject>P302</dc:subject>
                                              <dc:subject>ASTROPHYSICAL JOURNAL</dc:subject>
                                              <dc:subject>HRZ RD</dc:subject>
                                              <dc:subject>EVOLUTION</dc:subject>
                                          <dc:description>We 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>
                                                                  <dc:relation>info:eu-repo/grantAgreement/EC/FP7/283393//Advanced Radio Astronomy in Europe (RADIONET3)/</dc:relation>
                                                  <dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stu430</dc:relation>
                                          <dc:type>info:eu-repo/semantics/article</dc:type>
                                          <dc:source>Monthly Notices of the Royal Astronomical Society (0035-8711) vol.440(2014)</dc:source>
                                                      <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:language>eng</dc:language>
                                  <dc:audience>Researchers</dc:audience>
                                  <dc:format>application/pdf</dc:format>
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