J/MNRAS/477/2173 GRBs data (Song+, 2018)
Outflows from black hole hyperaccretion systems:
short and long-short gamma-ray bursts and 'quasi-supernovae'.
Song C.-Y., Liu T., Li A.
<Mon. Not. R. Astron. Soc., 477, 2173-2182 (2018)>
=2018MNRAS.477.2173S 2018MNRAS.477.2173S (SIMBAD/NED BibCode)
ADC_Keywords: GRB ; Accretion
Keywords: accretion, accretion discs - black hole physics - magnetic fields -
gamma-ray burst: general - stars: neutron
Abstract:
The detections of some long gamma-ray bursts (LGRBs) relevant to
mergers of neutron star (NS)-NS or black hole (BH)-NS, as well as some
short gamma-ray bursts (SGRBs) probably produced by collapsars, muddle
the boundary of two categories of gamma-ray bursts (GRBs). In both
cases, a plausible candidate of central engine is a BH surrounded by a
hyperaccretion disc with strong outflows, launching relativistic jets
driven by Blandford-Znajek mechanism. In the framework of compact
binary mergers, we test the applicability of the BH hyperaccretion
inflow-outflow model on powering observed GRBs. We find that, for a
low outflow ratio, ∼50 per cent, post-merger hyperaccretion processes
could power not only all SGRBs but also most of LGRBs. Some LGRBs
might originate from merger events in the BH hyperaccretion scenario,
at least on the energy requirement. Moreover, kilonovae might be
produced by neutron-rich outflows, and their luminosities and
time-scales significantly depend on the outflow strengths. GRBs and
their associated kilonovae are competitive with each other on the disc
mass and total energy budgets. The stronger the outflow, the more
similar the characteristics of kilonovae to supernovae (SNe). This
kind of 'nova' might be called 'quasi-SN'.
Description:
We collected the data of T90, z, Egamma,iso, Ek,iso, θj
and the peak energy in the rest frame Ep, rest of 30 SGRBs and 89
LGRBs.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 162 119 GRBs data
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Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 7 A7 --- Name GRB designation
8 A1 --- n_Name [*] Note on Name (1)
10- 17 F8.3 s T90 ? Duration
19- 24 F6.3 s e_T90 ? rms uncertainty on T90
26- 31 F6.4 --- z Redshift
34- 42 F9.5 10+45J Egiso Isotropic radiated energy of afterglow
(in 1052erg)
43 A1 --- --- [|+]
44- 51 F8.5 10+45J E_Egiso ? Error on Egiso (upper limit)
52 A1 --- --- [|-]
53- 60 F8.5 10+45J e_Egiso ? Error on Egiso (lower limit)
61- 62 A2 --- l_Ekiso [≤ ] Limit flag on Ekiso
63- 71 F9.4 10+45J Ekiso Iisotropic kinetic energy of afterglow
(in 1052erg)
72 A1 --- --- [|+]
73- 80 F8.3 10+45J E_Ekiso ? Error on Ekiso (upper limit)
81 A1 --- --- [|-]
82- 89 F8.3 10+45J e_Ekiso ? Error on Ekiso (upper limit)
91 A1 --- l_Eprest Limit flag on Eprest
92-100 F9.4 keV Eprest Peak energy in the rest frame
101 A1 --- --- [|+]
102-110 F9.4 keV E_Eprest ? Error on Eprest (upper limit)
111 A1 --- --- [|-]
112-120 F9.4 keV e_Eprest ? Error on Eprest (lower limit)
122 A1 --- l_thetaj Limit flag on thetaj
123-128 F6.4 rad thetaj Jet opening angle
129 A1 --- --- [|+]
130-135 F6.4 rad E_thetaj ? Error on thetaj (upper limit)
136 A1 --- --- [|-]
137-142 F6.4 rad e_thetaj ? Error on thetaj (lower limit)
143-152 F10.5 10+43W Lj Jet power (in 1050erg/s)
154-162 A9 --- Ref References (2)
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Note (1): * for GRBs that have unusual characteristics on observations
(Zhang et al., 2009ApJ...703.1696Z 2009ApJ...703.1696Z; Xin et al., 2011MNRAS.410...27X 2011MNRAS.410...27X).
Note (2): References as follows:
1 = Liu et al. (2015ApJS..218...12L 2015ApJS..218...12L)
2 = Butler et al. (2007ApJ...671..656B 2007ApJ...671..656B)
3 = Zhang et al. (PhD Thesis, Univ. Nevada, Las Vegas)
4 = Ryan et al. (2015ApJ...798....3Z 2015ApJ...798....3Z)
5 = Racusin et al. (2009ApJ...698...43R 2009ApJ...698...43R)
6 = Kann et al. (2011ApJ...734...96K 2011ApJ...734...96K)
7 = Zhang et al. (2012ApJ...750...88Z 2012ApJ...750...88Z)
8 = Antonelli et al. (2009A&A...507L..45A 2009A&A...507L..45A)
9 = Tsutsui et al. (2013MNRAS.431.1398T 2013MNRAS.431.1398T)
10 = Zaninoni et al. ((2016MNRAS.455.1375Z 2016MNRAS.455.1375Z)
11 = Berger et al. (2013ApJ...774L..23B 2013ApJ...774L..23B)
12 = Cummings et al. (2013GCN.15293....1C 2013GCN.15293....1C)
13 = Sakamoto et al. (2014GCN.16438....1S 2014GCN.16438....1S)
14 = Stanbro & Meegan (2016GCN.19843....1S 2016GCN.19843....1S)
15 = Lue et al. (2017ApJ...835..181L 2017ApJ...835..181L)
16 = Amati et al. (2008MNRAS.391..577A 2008MNRAS.391..577A)
17 = Song et al. (2016MNRAS.458.1921S 2016MNRAS.458.1921S)
18 = Nemmen et al. (2012Sci...338.1445N 2012Sci...338.1445N, Cat. J/other/Sci/338.1445)
19 = Yi et al. (2016ApJS..224...20Y 2016ApJS..224...20Y, Cat. J/ApJS/224/20)
20 = Zhang et al. ((2007ApJ...655..989Z 2007ApJ...655..989Z)
21 = Kann et al. (2010ApJ...720.1513K 2010ApJ...720.1513K, Cat. J/ApJ/720/1513)
22 = Xu et al. (2009ApJ...696..971X 2009ApJ...696..971X)
23 = Ofek et al. (2007ApJ...662.1129O 2007ApJ...662.1129O)
24 = Guidorzi et al. (2009A&A...499..439G 2009A&A...499..439G)
25 = Amati, Frontera & Guidorzi (2009A&A...508..173A 2009A&A...508..173A)
26 = Guidorzi et al. (2011MNRAS.417.2124G 2011MNRAS.417.2124G)
27 = Kruehler et al. (2009A&A...508..593K 2009A&A...508..593K, Cat. J/A+A/508/593)
28 = Dichiara et al. (2016A&A...589A..97D 2016A&A...589A..97D, Cat. J/A+A/589/A97)
29 = Ghirlanda et al. (2012MNRAS.420..483G 2012MNRAS.420..483G)
30 = Marshall et al. (2011ApJ...727..132M 2011ApJ...727..132M)
31 = Laskar et al. (2015ApJ...814....1L 2015ApJ...814....1L, Cat. J/ApJ/814/1)
32 = Gorbovskoy et al. (2012MNRAS.421.1874G 2012MNRAS.421.1874G, Cat. J/MNRAS/421/1874)
33 = Demianski et al. (2017A&A...598A.112D 2017A&A...598A.112D)
34 = Yasuda et al. ((2017MNRAS.466.4558Y 2017MNRAS.466.4558Y)
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History:
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(End) Patricia Vannier [CDS] 04-Jun-2021