Evidence for a proto-black hole and a double astrophysical component in GRB 101023
arXiv:1112.2970 · doi:10.1051/0004-6361/201118403
Abstract
[Shortened] Context: [...] we point out a striking similarity between GRB 101023 and GRB 090618. We explore the possibility that these sources are members of a new GRB family related to a single core-collapse. We use this understanding of the source in order to infer the unobserved redshift of GRB 101023. [...]. Aims: In precise analogy with GRB 090618 we aim to analyze the 89s of emission of GRB 101023 to see if we are in presence of two different episodes: the first one presenting a characteristic Black-body temperature evolution, evolving in time with a broken power-law, and the second one consistent with a canonical GRB. [...] Results: We confirm that the first episode can be well fit by a Black body plus a power-law model. The temperature changes with time following a broken power law, and the photon index of the power-law component presents a soft to hard evolution. We estimate the radius of this source, increasing with time with a velocity of 1.5x10^4 km/s. The second episode appears to be a canonical GRB. By using the Amati relation and the Atteia relation, we determine the cosmological redshift, z ~ 0.9 +- 0.084 (stat.) +- 0.2 (sys.). [...]. Particularly striking is the scaling law of the soft X-ray component of the afterglow. Conclusions: We identify GRB 090618 and GRB 101023 with a new family of GRBs presenting a double astrophysical component. A first one, related to the proto-black hole, prior to the process of gravitational collapse (episode 1) and a second one which is the canonical GRB (episode 2) emitted during the formation of the black-hole. [...] This analysis indicates progress towards developing a GRB distance indicator based on the understanding of the P-GRB and the prompt radiation as well as the soft X-Ray behavior of the late afterglow.
11 pages, 18 figures, accepted on A&A. New version fixing some typos. This is the version actually in press
References in corpus (9)
- An online repository of Swift/XRT light curves of GRBs
- A Photometric Redshift of z ~ 9.4 for GRB 090429B
- Quasi-blackbody component and radiative efficiency of the prompt emission of gamma-ray bursts
- A new method of determining the initial size and Lorentz factor of gamma-ray burst fireballs using a thermal emission component
- Intrinsic properties of a complete sample of HETE-2 gamma-ray bursts. A measure of the GRB rate in the Local Universe
- GRB060614: a "fake" short GRB from a merging binary system
- Redshift Filtering by Swift Apparent X-ray Column Density
- GRB 071227: an additional case of a disguised short burst
- On the nature of GRB 050509b: a disguised short GRB
Cited by in corpus (23)
- On the Induced Gravitational Collapse of a Neutron Star to a Black Hole by a Type Ib/c Supernova
- Hypercritical Accretion, Induced Gravitational Collapse, and Binary-Driven Hypernovae
- The ultra-long GRB 111209A - II. Prompt to afterglow and afterglow properties
- On the classification of GRBs and their occurrence rates
- A double component in GRB 090618: a proto-black hole and a genuinely long GRB
- Early X-ray Flares in GRBs
- GRB 090618: The First Example of a Neutron Star Gravitational Collapse to a Black Hole Induced by a Type Ib/c Supernova
- On Binary Driven Hypernovae and their nested late X-ray emission
- GRB 130427A and SN 2013cq: A Multi-wavelength Analysis of An Induced Gravitational Collapse Event
- GRB 090227B: the missing link between the genuine short and long GRBs
- Novel distance indicator for gamma-ray bursts associated with supernovae
- GRB 110709B in the Induced Gravitational Collapse paradigm
- Analysis of GRB 080319B and GRB 050904 within the fireshell model: evidence for a broader spectral energy distribution
- GRB 090510: a genuine short-GRB from a binary neutron star coalescing into a Kerr-Newman black hole
- On the ultra-relativistic Prompt Emission (UPE), the Hard and Soft X-ray Flares, and the extended thermal emission (ETE) in GRB 151027A
- Induced Gravitational Collapse, Binary-Driven Hypernovae, Long Gramma-ray Bursts and Their Connection with Short Gamma-ray Bursts
- Induced gravitational collapse at extreme cosmological distances: the case of GRB 090423
- Cooling of young neutron stars in GRB associated to Supernova
- GRB 081024B and GRB 140402A: two additional short GRBs from binary neutron star mergers
- On the universal late X-ray emission of binary-driven hypernovae and its possible collimation
- Induced Gravitational Collapse in the BATSE era: the case of GRB 970828
- GRB 090618: different pulse temporal and spectral characteristics within a burst
- A common behavior in the late X-ray afterglow of energetic GRB-SN systems