The metamorphosis of supernova SN 2008D/XRF 080109: A link between supernovae and GRBs/hypernovae

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The only supernovae (SNe) to show gamma-ray bursts (GRBs) or early x-ray emission thus far are overenergetic, broad-lined type Ic SNe (hypernovae, HNe). Recently, SN 2008D has shown several unusual features: (i) weak x-ray flash (XRF), (ii) an early, narrow optical peak, (iii) disappearance of the b...

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Autor principal: Mazzali, P.A
Otros Autores: Valenti, S., Della Valle, M., Chincarini, G., Sauer, D.N, Benetti, S., Pian, E., Piran, T., D'Elia, V., Elias-Rosa, N., Margutti, R., Pasotti, F., Antonelli, L.A, Bufano, F., Campana, S., Cappellaro, E., Covino, S., D'Avanzo, P., Fiore, F., Fugazza, D., Gilmozzi, R., Hunter, D., Maguire, K., Maiorano, E., Marziani, P., Masetti, N., Mirabel, F., Navasardyan, H., Nomoto, K., Palazzi, E., Pastorello, A., Panagia, N., Pellizza, L.J, Sari, R., Smartt, S., Tagliaferri, G., Tanaka, M., Taubenberger, S., Tominaga, N., Trundle, C., Turatto, M.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: 2008
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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030 |a SCIEA 
100 1 |a Mazzali, P.A. 
245 1 4 |a The metamorphosis of supernova SN 2008D/XRF 080109: A link between supernovae and GRBs/hypernovae 
260 |c 2008 
270 1 0 |m Mazzali, P. A.; Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany; email: mazzali@mpa-garching.mpg.de 
506 |2 openaire  |e Política editorial 
504 |a Berger, E., Soderberg, A.M., (2008), GCN 7159. , http://gcn.gsfc.nasa.gov/gcn3/7159.gcn3; Deng, J., Zhu, Y., (2008), GCN 7160. , http://gcn.gsfc.nasa.gov/gcn3/7160.gcn3; Valenti, S., (2008), GCN 7171. , http://gcn.gsfc.nasa.gov/gcn3/7171.gcn3; Filippenko, A.V., (1997) Annu. Rev. Astron. Astrophys, 35, p. 309 
504 |a Galama, T.J., (1998) Nature, 395, p. 670 
504 |a Iwamoto, K., (1998) Nature, 395, p. 672 
504 |a Pian, E., (2006) Nature, 442, p. 1011 
504 |a Mazzali, P.A., (2006) Nature, 442, p. 1018 
504 |a Mazzali, P.A., (2002) Astrophys. J, 572, pp. L61 
504 |a Fruchter, A.S., (2006) Nature, 441, p. 463 
504 |a Stritzinger, M., (2002) Astron. J, 124, p. 2100 
504 |a Modjaz, M., Chornock, R., Foley, R.J., Filippenko, A.V., Li, W., Stringfellow, G., (2008), GCN 7212. , http://gcn.gsfc.nasa.gov/gcn3/7212.gcn3; Mazzali, P.A., Iwamoto, K., Nomoto, K., (2000) Astrophys. J, 545, p. 407 
504 |a Tominaga, N., (2005) Astrophys. J, 633, pp. L97 
504 |a Mazzali, P.A., Lucy, L.B., (1998) Mon. Not. R. Astron. Soc, 295, p. 428 
504 |a Lucy, L.B., (1991) Astrophys. J, 383, p. 308 
504 |a Sauer, D., (2006) Mon. Not. R. Astron. Soc, 369, p. 1939 
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504 |a Maeda, K., Mazzali, P.A., Nomoto, K., (2006) Astrophys. J, 645, p. 1331 
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504 |a Soderberg, A.M., (2008) Nature, 453, p. 469 
504 |a Campana, S., (2006) Nature, 442, p. 1008 
504 |a Mazzali, P.A., (2005) Science, 308, p. 1284 
504 |a Maeda, K., (2008) Science, 319, p. 1220 
504 |a Bucciantini, N., (2008) Mon. Not. R. Astron. Soc, 383, pp. L2 
504 |a Arnett, W.D., (1982) Astrophys. J, 253, p. 785 
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520 3 |a The only supernovae (SNe) to show gamma-ray bursts (GRBs) or early x-ray emission thus far are overenergetic, broad-lined type Ic SNe (hypernovae, HNe). Recently, SN 2008D has shown several unusual features: (i) weak x-ray flash (XRF), (ii) an early, narrow optical peak, (iii) disappearance of the broad lines typical of SN Ic HNe, and (iv) development of helium lines as in SNe Ib. Detailed analysis shows that SN 2008D was not a normal supernova: Its explosion energy (E ≈ 6 × 10 51 erg) and ejected mass [∼7 times the mass of the Sun (M Fish eye )] are intermediate between normal SNe Ibc and HNe. We conclude that SN 2008D was originally a ∼30 M Fish eye 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.  |l eng 
536 |a Detalles de la financiación: Science and Technology Facilities Council, STFC, PP/C506805/1 
536 |a Detalles de la financiación: Science and Technology Facilities Council, STFC, PP/D508212/1 
536 |a Detalles de la financiación: Science and Technology Facilities Council, STFC, PP/E003303/1 
536 |a Detalles de la financiación: Science and Technology Facilities Council, STFC, ST/G000921/1 
593 |a Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Strasse 1, 85748 Garching, Germany 
593 |a Istituto Nazionale di Astrofisica-OAPd, vicolo dell'Osservatorio, 2, I-35122 Padova, Italy 
593 |a Department of Astronomy, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan 
593 |a Research Center for the Early Universe, School of Science, University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan 
593 |a Astrophysics Research Centre, School of Mathematics and Physics, Queen's University, Belfast, BT7 1NN, United Kingdom 
593 |a Dipartimento di Fisica, Universita di Ferrara, Via Giuseppe Saragat 1, 44100 Ferrara, Italy 
593 |a Istituto Nazionale di Astrofisica, Capodimonte Astronomical Observatory, Salita Moiariello 16, I-80131 Napoli, Italy 
593 |a European Southern Observatory, Karl-Schwarzschild-Strasse 2, D-85748 Garching, Germany 
593 |a International Center for Relativistic Astrophysics Network, Piazzale della Repubblica 10, I-65122 Pescara, Italy 
593 |a Department of Physics, Universita di Milano-Bicocca, Piazza delle Scienze 3, I-20126 Milano, Italy 
593 |a Istituto Nazionale di Astrofisica, Brera Astronomical Observatory, Via Emilio Bianchi 46, I-23807 Merate (LC), Italy 
593 |a Istituto Nazionale di Astrofisica-OATs, Via Tiepolo 11, I-34131 Trieste, Italy 
593 |a Racah Institute of Physics, Hebrew University, Jerusalem 91904, Israel 
593 |a Istituto Nazionale di Astrofisica, Rome Astronomical Observatory, Via di Frascati 33, I-00040 Monte Porzio Catone, Italy 
593 |a Istituto Nazionale di Astrofisica, Istituto di Astrofisica Spaziale e Fisica Cosmica, Via Piero Gobetti 101, I-40129 Bologna, Italy 
593 |a European Southern Observatory, Alonso de Cordova 3107, Santiago, Chile 
593 |a Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa, Chiba 277-8582, Japan 
593 |a Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States 
593 |a Istituto Nazionale di Astrofisica, Catania Astronomical Observatory, Via Santa Sofia 78, I-95123 Catania, Italy 
593 |a Instituto de Astronomía Y Física del Espacio, Casilla de Correos 67, Buenos Aires, Argentina 
690 1 0 |a HELIUM 
690 1 0 |a ASTRONOMY 
690 1 0 |a COSMOLOGY 
690 1 0 |a METAMORPHOSIS 
690 1 0 |a ARTICLE 
690 1 0 |a COSMOS 
690 1 0 |a EXPLOSION 
690 1 0 |a GAMMA RADIATION 
690 1 0 |a LUMINANCE 
690 1 0 |a PRIORITY JOURNAL 
690 1 0 |a SPACE 
690 1 0 |a X RAY ANALYSIS 
700 1 |a Valenti, S. 
700 1 |a Della Valle, M. 
700 1 |a Chincarini, G. 
700 1 |a Sauer, D.N. 
700 1 |a Benetti, S. 
700 1 |a Pian, E. 
700 1 |a Piran, T. 
700 1 |a D'Elia, V. 
700 1 |a Elias-Rosa, N. 
700 1 |a Margutti, R. 
700 1 |a Pasotti, F. 
700 1 |a Antonelli, L.A. 
700 1 |a Bufano, F. 
700 1 |a Campana, S. 
700 1 |a Cappellaro, E. 
700 1 |a Covino, S. 
700 1 |a D'Avanzo, P. 
700 1 |a Fiore, F. 
700 1 |a Fugazza, D. 
700 1 |a Gilmozzi, R. 
700 1 |a Hunter, D. 
700 1 |a Maguire, K. 
700 1 |a Maiorano, E. 
700 1 |a Marziani, P. 
700 1 |a Masetti, N. 
700 1 |a Mirabel, F. 
700 1 |a Navasardyan, H. 
700 1 |a Nomoto, K. 
700 1 |a Palazzi, E. 
700 1 |a Pastorello, A. 
700 1 |a Panagia, N. 
700 1 |a Pellizza, L.J. 
700 1 |a Sari, R. 
700 1 |a Smartt, S. 
700 1 |a Tagliaferri, G. 
700 1 |a Tanaka, M. 
700 1 |a Taubenberger, S. 
700 1 |a Tominaga, N. 
700 1 |a Trundle, C. 
700 1 |a Turatto, M. 
773 0 |d 2008  |g v. 321  |h pp. 1185-1188  |k n. 5893  |p Science  |x 00368075  |w (AR-BaUEN)CENRE-344  |t Science 
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856 4 0 |u https://doi.org/10.1126/science.1158088  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_00368075_v321_n5893_p1185_Mazzali  |y Handle 
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