2014ApJ...786L...8W

Query : 2014ApJ...786L...8W

2014ApJ...786L...8W - Astrophys. J., 786, L8 (2014/May-1)

Similar radiation mechanism in gamma-ray bursts and blazars: evidence from two luminosity correlations.

WANG F.Y., YI S.X. and DAI Z.G.

Abstract (from CDS):

Active galactic nuclei and gamma-ray bursts (GRBs) are powerful astrophysical events with relativistic jets. In this Letter, the broadband spectral properties of GRBs and well-observed blazars are compared. The distribution of GRBs is consistent with the well-known blazar sequence including the νLν(5 GHz) - αRX and νLν(5 GHz) - νpeakcorrelations, where αRXis defined as the broadband spectral slope in radio-to-X-ray bands, and νpeakis defined as the spectral peak frequency. Moreover, GRBs occupy the low radio luminosity end of these sequences. These two correlations suggest that GRBs could have a radiation process, i.e., synchrotron radiation, similar to blazars both in the prompt emission and afterglow phases.

Abstract Copyright: ∼

Journal keyword(s): BL Lacertae objects: general - gamma-ray burst: general - methods: statistical

Simbad objects: 43

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Number of rows : 43
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 021004 gB 00 26 54.68 +18 55 41.6           ~ 560 0
2 GRB 050824 gB 00 48 56.100 +22 36 32.00 19.66 21.03 20.46 23.70   ~ 184 0
3 GRB 050904 gB 00 54 50.794 +14 05 09.42           ~ 496 0
4 Fermi bn100814160 gB 01 29 53.61 -17 59 43.6           ~ 219 0
5 GRB 100901A gB 01 49 03.56 +22 45 30.6           ~ 170 0
6 GRB 100906A gB 01 54 44.19 +55 37 49.8           ~ 233 0
7 GRB 000210 gB 01 59 15 -40 40.0           ~ 175 0
8 GRB 050603 gB 02 39 56.839 -25 10 54.92     18.48     ~ 174 0
9 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 1007 1
10 GRB 991216 gB 05 09 31.2983 +11 17 07.262           ~ 430 0
11 GRB 090328 gB 06 02 39.69 -41 52 55.1           ~ 194 1
12 GRB 970508 gB 06 53 49.2 +79 16 19           ~ 883 1
13 GRB 980329 gB 07 02 41 +38 50.7           ~ 276 1
14 GRB 070125 gB 07 51 17.80 +31 09 04.8           ~ 188 0
15 GRB 071020 gB 07 58 39.65 +32 51 38.8           ~ 158 0
16 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 576 0
17 Fermi bn090423330 gB 09 55 33.19 +18 08 57.7           ~ 392 0
18 GRB 071010B gB 10 02 09.20 +45 43 52.2           ~ 173 0
19 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1261 1
20 GRB 030226 gB 11 33 04.9 +25 53 56           ~ 212 0
21 GRB 011121 gB 11 34 26.67 -76 01 41.6       23.0   ~ 286 1
22 Fermi bn091020900 gB 11 42 55.20 +50 58 42.0           ~ 188 0
23 GRB 050416 gB 12 33 54.600 +21 03 26.69     19.12     ~ 300 1
24 GRB 090424 gB 12 38 07.40 +16 49 45.9           ~ 269 0
25 Fermi bn090323002 gB 12 42 50.28 +17 03 11.9           ~ 244 1
26 Fermi bn100414097 gB 12 48 30.0 +08 41 35           ~ 136 0
27 GRB 090313 gB 13 13 36.00 +08 05 10.7           ~ 149 0
28 GRB 990510 gB 13 38 07.64 -80 29 48.8           ~ 499 1
29 GRB 050730 gB 14 08 17.090 -03 46 18.90   20.32 17.68     ~ 327 0
30 GRB 010222 G 14 52 12.5 +43 01 06           ~ 364 1
31 GRB 060418 gB 15 45 42.600 -03 38 20.00 15.73 16.19 14.98     ~ 389 0
32 GRB 050401 gB 16 31 28.84 +02 11 14.5           ~ 348 0
33 GRB 090715B gB 16 45 21.59 +44 50 20.1           ~ 144 0
34 GRB 100418A gB 17 05 26.96 +11 27 41.9           ~ 198 0
35 Fermi bn090902462 gB 17 39 45.26 +27 19 28.1           ~ 440 0
36 GRB 970828 gB 18 08 31.6 +59 18 51           ~ 353 1
37 SN 2005nc SN* 18 32 32.560 +26 20 22.34           SNIc: 400 1
38 GRB 080603A gB 18 37 37.95 +62 44 39.6           ~ 89 0
39 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1928 2
40 GRB 071003 gB 20 07 24.50 +10 56 48.8           ~ 181 0
41 GRB 050820A gB 22 29 38.110 +19 33 37.10 18.33 19.00 18.47     ~ 409 0
42 GRB 051022A gB 23 56 04.200 +19 36 32.30           ~ 194 1
43 GRB 980703 gB 23 59 06.7 +08 35 07           ~ 453 1

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