An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova
Gamma-ray bursts (GRBs) are short, intense flashes of soft γ-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ∼2 s) are believed to originate from the deaths of massive stars, mainly on the basis of a handful of solid associations between GRBs and supernovae. GRB 06...
Guardado en:
| Autor principal: | |
|---|---|
| Otros Autores: | , , , , , , , , , , , , , , , |
| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
Nature Publishing Group
2006
|
| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
| Aporte de: | Registro referencial: Solicitar el recurso aquí |
| LEADER | 09304caa a22011297a 4500 | ||
|---|---|---|---|
| 001 | PAPER-21676 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230518205309.0 | ||
| 008 | 190411s2006 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-33845873615 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 030 | |a NATUA | ||
| 100 | 1 | |a Valle, M.D. | |
| 245 | 1 | 3 | |a An enigmatic long-lasting γ-ray burst not accompanied by a bright supernova |
| 260 | |b Nature Publishing Group |c 2006 | ||
| 270 | 1 | 0 | |m Valle, M.D.; INAF, Osservatorio Astrofisico di Arcetri, largo E. Fermi 5, I-50125 Firenze, Italy; email: massimo@arcetri.astro.it |
| 506 | |2 openaire |e Política editorial | ||
| 504 | |a Woosley, S.E., Bloom, J.S., The supernova-gamma-ray burst connection (2006) Annu. Rev. Astron. Astrophys, 44, pp. 507-556 | ||
| 504 | |a Galama, T.J., An unusual supernova in the error box of the γ-ray burst of 25 April 1998 (1998) Nature, 395, pp. 670-672 | ||
| 504 | |a Stanek, K.Z., Spectroscopic discovery of the supernova 2003dh associated with GRB 030329 (2003) Astrophys. J, 591, pp. L17-L20 | ||
| 504 | |a Hjorth, J., A very energetic supernova associated with the γ-ray burst of 29 March 2003 (2003) Nature, 423, pp. 847-850 | ||
| 504 | |a Malesani, D., SN 2003lw and GRB 031203: A bright supernova for a faint gamma-ray burst (2004) Astrophys. J, 609, pp. L5-L8 | ||
| 504 | |a Pian, E., An optical supernova associated with the X-ray flash XRF 060218 (2006) Nature, 442, pp. 1011-1013 | ||
| 504 | |a Campana, S., The association of GRB 060218 with a supernova and the evolution of the shock wave (2006) Nature, 442, pp. 1008-1010 | ||
| 504 | |a Gehrels, N., A new γ-ray burst classification scheme from GRB 060614 Nature, , doi:10.1038/nature05376 this issue | ||
| 504 | |a Parsons, A.M., GRB 060614: Swift detection of a burst with a bright optical and X-ray counterpart (2006) GCN Circ, 5252 | ||
| 504 | |a Ferrero, P., The GRB 060218/SN 2006aj event in the context of other gamma-ray burst supernovae (2006) Astron. Astrophys, 457, pp. 857-864 | ||
| 504 | |a Christensen, L., Hjorth, J., Gorosabel, J., UV star-formation rates of GRB host galaxies (2004) Astron. Astrophys, 425, pp. 913-926 | ||
| 504 | |a Fruchter, A.S., Long γ-ray bursts and core-collapse supernovae have different environments (2006) Nature, 441, pp. 463-468 | ||
| 504 | |a Gal-Yam, A., A novel explosive process is required for the γ-ray burst GRB 060614 Nature, , doi:10.1038/nature05373 this issue | ||
| 504 | |a Fynbo, J.P.U., No supernovae associated with two long-lasting γ-ray bursts Nature, , doi:10.1038/nature05375 this issue | ||
| 504 | |a Patat, F., The metamorphosis of SN 1998bw (2001) Astrophys. J, 555, pp. 900-917 | ||
| 504 | |a Foley, R., Optical photometry and spectroscopy of the SN 1998bw-like type Ic supernova 2002ap (2003) Publ. Astron. Soc. Pacif, 115, pp. 1220-1235 | ||
| 504 | |a Romaniello, M., Panagia, N., Scuderi, S., Kirshner, R.P., Accurate stellar population studies from multiband photometric observations (2002) Astron. J, 123, pp. 915-940 | ||
| 504 | |a Della Valle, M., Hypernova signatures in the late rebrightening of GRB 050525A (2006) Astrophys. J, 642, pp. L103-L106 | ||
| 504 | |a Hamuy, M., Observed and physical properties of core-collapse supernovae (2003) Astrophys. J, 582, pp. 905-914 | ||
| 504 | |a Panagia, N. in Supernovae and Gamma-Ray Bursters (ed. Weiler, K. W.) 113-144 (Lecture Notes in Physics, 598, Springer, Berlin, 2003); Pastorello, A., Low luminosity type II supernovae: Spectroscopic and photometric evolution (2004) Mon. Not. R. Astron. Soc, 347, pp. 74-94 | ||
| 504 | |a Nomoto, K. et al. in Stellar Collapse (ed. Fryer, C.) 277-325 (Astrophysics and Space Science Library, 302, Kluwer Academic, Dordrecht, 2004); Eichler, D., Livio, M., Piran, T., Schramm, D.N., Nucleosynthesis, neutrino bursts and γ-rays from coalescing neutron stars (1989) Nature, 340, pp. 126-128 | ||
| 504 | |a Blinnikov, S. I. & Postnov, K. A. A mini-SN model for optical afterglow of GRBs. Mon. Not. R. Astron. Soc. 293, L29-L32 (1998); Vietri, M., Stella, L.A., Gamma-ray burst model with small baryon contamination (1998) Astrophys. J, 507, pp. L45-L48 | ||
| 504 | |a Belczynski, K., Bulik, T., Rudak, B., Study of gamma-ray burst binary progenitors (2002) Astrophys. J, 571, pp. 394-412 | ||
| 504 | |a Woosley, S.E., Zhang, W., Heger, A., Gamma-Ray Burst and Afterglow Astronomy 2001: A Workshop Celebrating the First Year of the HETE Mission (2003) 185-192 (AIP Conf. Proc, 662. , eds Ricker, G. R. & Vanderspek, R, American Institute of Physics, New York | ||
| 504 | |a Price, P.A., Berger, E., Fox, D.B., GRB 060614: Redshift (2006) GCN Circ, 5275 | ||
| 504 | |a French, F., Melady, G., Hanlon, L., Jelínek, M., Kubánek, P., GRB060614: Watcher observation (2006) GCN Circ, 5257 | ||
| 520 | 3 | |a Gamma-ray bursts (GRBs) are short, intense flashes of soft γ-rays coming from the distant Universe. Long-duration GRBs (those lasting more than ∼2 s) are believed to originate from the deaths of massive stars, mainly on the basis of a handful of solid associations between GRBs and supernovae. GRB 060614, one of the closest GRBs discovered, consisted of a 5-s hard spike followed by softer, brighter emission that lasted for ∼100 s (refs 8, 9). Here we report deep optical observations of GRB 060614 showing no emerging supernova with absolute visual magnitude brighter than MV = -13.7. Any supernova associated with GRB 060614 was therefore at least 100 times fainter, at optical wavelengths, than the other supernovae associated with GRBs. This demonstrates that some long-lasting GRBs can either be associated with a very faint supernova or produced by different phenomena. ©2006 Nature Publishing Group. |l eng | |
| 536 | |a Detalles de la financiación: Agenzia Spaziale Italiana | ||
| 536 | |a Detalles de la financiación: Acknowledgements This work is based on data collected at the Very Large Telescope operated by the European Southern Observatory. We acknowledge support from the observing staff. This research is supported in Italy by ASI, MIUR-PRIN and INAF-PRIN grants. | ||
| 593 | |a INAF, Osservatorio Astrofisico di Arcetri, largo E. Fermi 5, I-50125 Firenze, Italy | ||
| 593 | |a Dipartimento di Fisica, Università degli Studi di Milano-Bicocca, piazza delle Scienze 3, I-20126 Milano, Italy | ||
| 593 | |a INAF, Osservatorio Astronomico di Brera, via E. Bianchi 46, I-23807 Merate (Lc), Italy | ||
| 593 | |a Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States | ||
| 593 | |a Istituto Nazionale di Astrofisica, viale del Parco Mellini 84, I-00136, Roma, Italy | ||
| 593 | |a Supernova Ltd., O. Yard Village #131, Northsound Rd., Virgin Gorda, Virgin Islands (British) | ||
| 593 | |a International School for Advanced Studies (SISSA/ISAS), via Beirut 2-4, I-34014 Trieste, Italy | ||
| 593 | |a INAF, Osservatorio Astronomico di Roma, via di Frascati 33, I-00040 Monteporzio Catone (Roma), Italy | ||
| 593 | |a INAF, Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo, via U. La Malfa 153, I-90146 Palermo, Italy | ||
| 593 | |a ASI Science Data Center, via G. Galilei, I-00044 Frascati, Italy | ||
| 593 | |a Dipartimento di Fisica e Matematica, Università dell'Insubria, via Valleggio 11, I-22100 Como, Italy | ||
| 593 | |a University of California, Berkeley, Space Sciences Laboratory, Berkeley, CA 94720-7450, United States | ||
| 593 | |a European Southern Observatory, A. C. 3107, Vitacura, Casilla 19001, Santiago 19, Chile | ||
| 593 | |a Instituto de Astronomía Y Física del Espacio (CONICET/UBA), Casilla de Correos 67 Suc. 28, (1428) Buenos Aires, Argentina | ||
| 690 | 1 | 0 | |a ASTROPHYSICS |
| 690 | 1 | 0 | |a GAMMA RAY RADIATION |
| 690 | 1 | 0 | |a OPTICAL METHOD |
| 690 | 1 | 0 | |a ARTICLE |
| 690 | 1 | 0 | |a COSMIC RADIATION |
| 690 | 1 | 0 | |a COSMOS |
| 690 | 1 | 0 | |a GAMMA RADIATION |
| 690 | 1 | 0 | |a LIGHT |
| 690 | 1 | 0 | |a LUMINANCE |
| 690 | 1 | 0 | |a PHOTOMETRY |
| 690 | 1 | 0 | |a PRIORITY JOURNAL |
| 690 | 1 | 0 | |a X RAY |
| 700 | 1 | |a Chincarini, G. | |
| 700 | 1 | |a Panagia, N. | |
| 700 | 1 | |a Tagliaferri, G. | |
| 700 | 1 | |a Malesani, D. | |
| 700 | 1 | |a Testa, V. | |
| 700 | 1 | |a Fugazza, D. | |
| 700 | 1 | |a Campana, S. | |
| 700 | 1 | |a Covino, S. | |
| 700 | 1 | |a Mangano, V. | |
| 700 | 1 | |a Antonelli, L.A. | |
| 700 | 1 | |a D'Avanzo, P. | |
| 700 | 1 | |a Hurley, K. | |
| 700 | 1 | |a Mirabel, I.F. | |
| 700 | 1 | |a Pellizza, L.J. | |
| 700 | 1 | |a Piranomonte, S. | |
| 700 | 1 | |a Stella, L. | |
| 773 | 0 | |d Nature Publishing Group, 2006 |g v. 444 |h pp. 1050-1052 |k n. 7122 |p Nature |x 00280836 |w (AR-BaUEN)CENRE-48 |t Nature | |
| 856 | 4 | 1 | |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-33845873615&doi=10.1038%2fnature05374&partnerID=40&md5=6a721794a44eff1c16e95d60cd8f7d30 |y Registro en Scopus |
| 856 | 4 | 0 | |u https://doi.org/10.1038/nature05374 |y DOI |
| 856 | 4 | 0 | |u https://hdl.handle.net/20.500.12110/paper_00280836_v444_n7122_p1050_Valle |y Handle |
| 856 | 4 | 0 | |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00280836_v444_n7122_p1050_Valle |y Registro en la Biblioteca Digital |
| 961 | |a paper_00280836_v444_n7122_p1050_Valle |b paper |c PE | ||
| 962 | |a info:eu-repo/semantics/article |a info:ar-repo/semantics/artículo |b info:eu-repo/semantics/publishedVersion | ||
| 963 | |a VARI | ||
| 999 | |c 82629 | ||