101. The Metamorphosis of Supernova SN 2008D/XRF 080109: A Link Between Supernovae and GRBs/Hypernovae
- Author
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Gianpiero Tagliaferri, N. Masetti, F. Pasotti, Nancy Elias-Rosa, Kate Maguire, Filomena Bufano, Leonardo J. Pellizza, Daniel Sauer, Enrico Cappellaro, Tsvi Piran, Masaomi Tanaka, Stefano Valenti, Andrea Pastorello, Sergio Campana, Fabrizio Fiore, Stephen Smartt, Stefano Benetti, H. Navasardyan, Carrie Trundle, P. D'Avanzo, Stefan Taubenberger, Paola Marziani, Valerio D'Elia, Eliana Palazzi, Raffaella Margutti, Ken'ichi Nomoto, Elena Pian, Roberto Gilmozzi, D. J. Hunter, Guido Chincarini, Stefano Covino, L. Angelo Antonelli, Massimo Turatto, Nozomu Tominaga, Dino Fugazza, Massimo Della Valle, Elisabetta Maiorano, Paolo A. Mazzali, F. Mirabel, Re'em Sari, and Nino Panagia
- Subjects
Physics ,Solar mass ,Multidisciplinary ,Ciencias Físicas ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astronomy ,chemistry.chemical_element ,purl.org/becyt/ford/1.3 [https] ,Astrophysics ,Astronomía ,BURSTS [GAMMA RAYS] ,purl.org/becyt/ford/1 [https] ,Black hole ,Stars ,Supernova ,Astrophysical jet ,chemistry ,Hypernova ,CIENCIAS NATURALES Y EXACTAS ,Helium - Abstract
The only supernovae (SNe) to have shown early gamma-ray or X-ray emission thus far are overenergetic, broad-lined Type Ic SNe (Hypernovae - HNe). Recently, SN 2008D shows several novel features: (i) weak XRF, (ii) an early, narrow optical peak, (iii) disappearance of the broad lines typical of SNIc HNe, (iv) development of He lines as in SNeIb. Detailed analysis shows that SN 2008D was not a normal SN: its explosion energy (KE ~ 6*10^{51} erg) and ejected mass (~7 Msun) are intermediate between normal SNeIbc and HNe. We derive that SN 2008D was originally a ~30Msun star. When it collapsed a black hole formed and a weak, mildly relativistic jet was produced, which caused the XRF. SN 2008D is probably among the weakest explosions that produce relativistic jets. Inner engine activity appears to be present whenever massive stars collapse to black holes., Comment: 22 pages, 7 figures. Accepted for publication in Science
- Published
- 2008
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