2021MNRAS.504.5301R

Query : 2021MNRAS.504.5301R

2021MNRAS.504.5301R - Mon. Not. R. Astron. Soc., 504, 5301-5326 (2021/July-2)

The morphology of the X-ray afterglows and of the jetted GeV emission in long GRBs.

RUFFINI R., MORADI R., RUEDA J.A., LI L., SAHAKYAN N., CHEN Y.-C., WANG Y., AIMURATOV Y., BECERRA L., BIANCO C.L., CHERUBINI C., FILIPPI S., KARLICA M., MATHEWS G.J., MUCCINO M., PISANI G.B. and XUE S.S.

Abstract (from CDS):

We recall evidence that long gamma-ray bursts (GRBs) have binary progenitors and give new examples. Binary-driven hypernovae (BdHNe) consist of a carbon-oxygen core (COcore) and a neutron star (NS) companion. For binary periods ∼5 min, the COcore collapse originates the subclass BdHN I characterized by (1) an outstanding supernova (SN; the 'SN-rise'); (2) a black hole (BH), born from the NS collapse by SN matter accretion, leading to a GeV emission with luminosity LGeV = AGeV t–\alphaGeV, observed only in some cases; and (3) a new NS (νNS), born from the SN, originating from the X-ray afterglow with LX = AX t–αX_^, observed in all BdHN I. We record 378 sources and present for four prototype GRBs 130427A, 160509A, 180720B, and 190114C: (1) spectra, luminosities, SN-rise duration; (2) AX, αX = 1.48 ± 0.32, and (3) the νNS spin time evolution. We infer (i) AGeV, αGeV = 1.19 ± 0.04 and (ii) the BdHN I morphology from time-resolved spectral analysis, three-dimensional simulations, and the GeV emission presence/absence in 54 sources within the Fermi-Large Area Telescope boresight angle. For 25 sources, we give the integrated and time-varying GeV emission, 29 sources have no GeV emission detected and show X/gamma-ray flares previously inferred as observed along the binary plane. The 25/54 ratio implies the GeV radiation is emitted within a cone of half-opening angle ≃60° from the normal to the orbital plane. We deduce BH masses of 2.3-8.9 M☉ and spin of 0.27-0.87 by explaining the GeV emission from the BH rotational energy extraction, while their time evolution validates the BH mass-energy formula.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): black hole physics - binaries: general - gamma-ray bursts - transients: supernovae

Simbad objects: 71

goto Full paper

goto View the references in ADS

Number of rows : 71
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 GRB 180720B gB 00 02 06.99 -02 55 07.8           ~ 215 0
2 Fermi bn180703876 gB 00 25 52.72 -67 10 47.9           ~ 35 0
3 Fermi bn131231198 gB 00 42 44.0 -01 29 40           ~ 103 0
4 Fermi bn140703026 gB 00 51 58.99 +45 06 05.4           ~ 90 0
5 GRB 081222 gB 01 30 57.76 -34 05 44.0           ~ 199 0
6 3B 940217 gB 01 56.3 +04 33           ~ 204 0
7 Fermi bn091208410 gB 01 57 38.50 +16 52 50.7           ~ 220 0
8 SN 2009nz SN* 02 26 19.87 -18 57 08.6           ~ 307 1
9 Fermi bn130925164 gB 02 44 42.38 -26 09 15.8           ~ 184 0
10 Fermi bn100728439 gB 02 56 13.44 +00 16 51.6           ~ 142 0
11 SN 2019oyw SN* 02 58 10.510 -08 57 27.20           ~ 218 0
12 GRB 140907A gB 03 12 34.98 +46 36 17.2           ~ 81 0
13 IC 310 AGN 03 16 42.9787569912 +41 19 29.615579544   14.3       ~ 311 2
14 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
15 GRB 190114C gB 03 38 01.18 -26 56 47.8           ~ 343 0
16 Fermi bn151111356 gB 03 47 22.76 -44 09 41.4           ~ 42 0
17 Fermi bn131105087 gB 04 43 53.50 -63 00 17.7           ~ 95 0
18 Fermi bn150514774 gB 04 59 30.45 -60 58 07.0           ~ 51 0
19 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 650 1
20 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
21 1B 910503 gB 05 49.8 +38 44           ~ 133 0
22 Fermi bn100728095 gB 05 55 02.00 -15 15 20.2           ~ 157 0
23 Fermi bn150301818 gB 05 56 40.04 -57 58 10.4           ~ 67 0
24 GRB 090328 gB 06 02 39.69 -41 52 55.1           ~ 194 1
25 GRB 970508 gB 06 53 49.2 +79 16 19           ~ 883 1
26 3B 940301 gB 06 54.0 +64 21           ~ 70 0
27 GRB 140213A gB 07 00 37.18 -73 08 14.1           ~ 102 0
28 GRB 080916C gB 07 59 23.24 -56 38 16.8           ~ 386 0
29 Fermi bn120119170 gB 08 00 06.940 -09 04 53.83           ~ 193 0
30 Fermi bn150314205 gB 08 26 40.82 +63 50 03.4           ~ 117 0
31 Fermi bn090516353 gB 09 12 59 -11 50.9           ~ 173 0
32 Fermi bn130528695 gB 09 18 00.12 +87 18 03.7           ~ 48 0
33 Fermi bn140206304 gB 09 41 16.90 +66 45 42.7           ~ 149 0
34 GRB 171222A gB 09 53 06.69 +35 37 36.1           ~ 57 0
35 Fermi bn111228657 gB 10 00 16.04 +18 17 52.2           ~ 201 0
36 GRB 131108A gB 10 26 00.480 +09 39 44.05           ~ 96 0
37 Fermi bn120712571 gB 11 18 21.16 -20 02 01.1           ~ 90 0
38 V* V779 Cen HXB 11 21 15.0920532528 -60 37 25.630264596   14.4 12.27     O9III/Veq 1159 0
39 Fermi bn120624933 gB 11 23 31.98 +08 55 42.1           ~ 100 0
40 SN 2013cq SN* 11 32 32.84 +27 41 56.2           SNIc 613 1
41 Fermi bn100615083 gB 11 48 49.25 -19 28 52.2           ~ 133 0
42 2B 930131 gB 12 08.2 -08 14           ~ 127 0
43 GRB 090424 gB 12 38 07.40 +16 49 45.9           ~ 269 0
44 Fermi bn090323002 gB 12 42 50.28 +17 03 11.9           ~ 244 1
45 Fermi bn100414097 gB 12 48 30.0 +08 41 35           ~ 136 0
46 Fermi bn110128073 gB 12 55 35.10 +28 03 54.1           ~ 80 0
47 Fermi bn141220252 gB 13 00 15.70 +32 08 47.2           ~ 81 0
48 Fermi bn140423356 gB 13 09 06.20 +49 50 18.3           ~ 114 0
49 Fermi bn170405777 gB 14 39 18.66 -25 14 36.9           ~ 75 0
50 Fermi bn140623224 gB 15 01 53.41 +81 11 29.0           ~ 34 0
51 GRB 091003A gB 16 46 04.680 +36 37 31.08           ~ 135 0
52 SN 2018fip SN* 16 54 15.64 -54 02 39.5           SNIc-BL 83 0
53 V* HZ Her LXB 16 57 49.8110126616 +35 20 32.486555472 11.90 14.89 13.63 13.88   B3/6ep 2172 0
54 GRB 170214A gB 17 05 21.94 -01 53 14.9           ~ 54 0
55 Fermi bn090902462 gB 17 39 45.26 +27 19 28.1           ~ 440 0
56 Fermi bn151027166 gB 18 09 56.87 +61 21 12.3           ~ 143 0
57 GRB 120909A gB 18 22 56.81 -59 26 54.9           ~ 103 0
58 Fermi bn110731465 gB 18 42 00.99 -28 32 13.8           ~ 193 0
59 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
60 GRB 160625B gB 20 34 23.67 +06 55 11.1           ~ 235 0
61 1B 910601 gB 20 40.5 +32 20           ~ 94 0
62 GRB 150403A gB 20 46 01.17 -62 42 40.1           ~ 116 0
63 Fermi bn160509374 gB 20 47 00.90 +76 06 30.1           ~ 141 0
64 Fermi bn120716712 gB 20 52 12.17 +09 35 53.9           ~ 72 0
65 GRB 141028A gB 21 30 24.46 -00 13 55.6           ~ 109 0
66 GRB 080514B gB 21 31 22.61 +00 42 30.3           ~ 69 0
67 GRB 161014A gB 22 10 35.42 +07 28 07.6           ~ 69 0
68 Fermi bn090510016 G 22 14 12.6230 -26 34 58.550           ~ 548 0
69 Fermi bn150821406 gB 22 47 39.15 -57 53 38.2           ~ 71 0
70 Fermi bn090926181 gB 23 33 36.18 -66 19 25.9           ~ 339 0
71 GRB 130518A gB 23 42 39.79 +47 27 55.2           ~ 86 0

To bookmark this query, right click on this link: simbad:objects in 2021MNRAS.504.5301R and select 'bookmark this link' or equivalent in the popup menu