2007
DOI: 10.1051/0004-6361:20078068
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GRB 060218 and GRBs associated with supernovae Ib/c

Abstract: Context. The Swift satellite has given continuous data in the range 0.3-150 keV from 0 s to 10 6 s for GRB 060218 associated with SN2006aj. This Gamma-Ray Burst (GRB) which has an unusually long duration (T 90 ∼ 2100 s) fulfills the Amati relation. These data offer the opportunity to probe theoretical models for GRBs connected with Supernovae (SNe). Aims. We plan to fit the complete γ-and X-ray light curves of this long duration GRB, including the prompt emission, in order to clarify the nature of the progenit… Show more

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Cited by 36 publications
(67 citation statements)
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“…We recall that the fireshell model (Damour & Ruffini 1975;Ruffini et al 2000Ruffini et al , 2010Ruffini 2001) is an alternative to the Fireball model, first proposed by Cavallo & Rees (1978), Goodman (1986) and Paczynsky (1986). We assume, within the fireshell model, that all GRBs originate from the gravitational collapse of a star approaching asymptotically the formation of a Kerr-Newmann BH (Wiltshire et al 2009).…”
Section: Analysis Of Episode 2 In the Fireshell Modelmentioning
confidence: 99%
“…We recall that the fireshell model (Damour & Ruffini 1975;Ruffini et al 2000Ruffini et al , 2010Ruffini 2001) is an alternative to the Fireball model, first proposed by Cavallo & Rees (1978), Goodman (1986) and Paczynsky (1986). We assume, within the fireshell model, that all GRBs originate from the gravitational collapse of a star approaching asymptotically the formation of a Kerr-Newmann BH (Wiltshire et al 2009).…”
Section: Analysis Of Episode 2 In the Fireshell Modelmentioning
confidence: 99%
“…Typical values of R ranges between 10 −10 and 10 −6 (see e.g. Bernardini et al 2007Bernardini et al , 2005Caito et al 2009Caito et al , 2010Dainotti et al 2007;Ruffini et al 2006).…”
Section: The Fireshell Modelmentioning
confidence: 99%
“…This second parameter takes into account the CBM filamentary structure (Ruffini et al 2004) and the possible occurrence of fragmentation in the shell (Dainotti et al 2007). The emission from the baryonic matter shell is spherically symmetric.…”
Section: Brief Summary Of the Fireshell Modelmentioning
confidence: 99%