2018A&A...616A.169M


C.D.S. - SIMBAD4 rel 1.7 - 2020.07.08CEST02:57:19

2018A&A...616A.169M - Astronomy and Astrophysics, volume 616A, 169-169 (2018/8-1)

The second-closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environment.

MICHALOWSKI M.J., XU D., STEVENS J., LEVAN A., YANG J., PARAGI Z., KAMBLE A., TSAI A.-L., DANNERBAUER H., VAN DER HORST A.J., SHAO L., CROSBY D., GENTILE G., STANWAY E., WIERSEMA K., FYNBO J.P.U., TANVIR N.R., KAMPHUIS P., GARRETT M. and BARTCZAK P.

Abstract (from CDS):

We report the detection of the radio afterglow of a long gamma-ray burst (GRB) 111005A at 5-345GHz, including very long baseline interferometry observations with a positional error of 0.2 mas. The afterglow position is coincident with the disc of a galaxy ESO 58049 at z=0.01326 (∼1'' from its centre), which makes GRB 111005A the second-closest GRB known to date, after GRB 980425. The radio afterglow of GRB 111005A was an order of magnitude less luminous than those of local low-luminosity GRBs, and obviously less luminous than those of cosmological GRBs. The radio flux was approximately constant and then experienced an unusually rapid decay a month after the GRB explosion. Similarly to only two other GRBs, we did not find the associated supernovae (SNe), despite deep near- and mid-infrared observations 1-9 days after the GRB explosion, reaching ∼20 times fainter than other SNe associated with GRBs. Moreover, we measured a twice-solar metallicity for the GRB location. The low y-ray and radio luminosities, rapid decay, lack of a SN, and super-solar metallicity suggest that GRB 111005A represents a rare class of GRB that is different from typical core-collapse events. We modelled the spectral energy distribution of the GRB 111005A host finding that it is a moderately star-forming dwarf galaxy, similar to the host of GRB 980425. The existence of two local GRBs in such galaxies is still consistent with the hypothesis that the GRB rate is proportional to the cosmic star formation rate (SFR) density, but suggests that the GRB rate is biased towards low SFRs. Using the far-infrared detection of ESO 580-49, we conclude that the hosts of both GRBs 111005A and 980425 exhibit lower dust content than what would be expected from their stellar masses and optical colors.

Abstract Copyright: © ESO 2018

Journal keyword(s): dust, extinction - galaxies: abundances - galaxies: individual: ESO 580-49 - galaxies: star formation - gamma-ray burst: general - gamma-ray burst: individual: 111005A

CDS comments: Paragraph. 1 EVLA-S1 not identified.

Simbad objects: 29

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Number of rows : 29

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 GRB 000210 gB 01 59 15 -40 40.0           ~ 164 0
2 SN 2006aj SN* 03 21 39.670 +16 52 02.27 17.96 19.11 17.40     SNIc-BL 828 1
3 NAME LMC G 05 23 34.6 -69 45 22     0.4     ~ 14826 1
4 SN 2010bh SN* 07 10 30.63 -56 15 19.7           SNIc 230 1
5 SN 2003lw SN* 08 02 30.1 -39 51 03       20.23   SNIc: 506 0
6 GRB 070306 gB 09 52 23.220 +10 28 55.20           ~ 177 1
7 GRB 980613 gB 10 17 57.8 +71 27 26           ~ 198 1
8 SN 2003dh SN* 10 44 50.030 +21 31 18.15     16.2     SNIcpec 1117 2
9 GRB 000418 gB 12 25 21 +20 05.0           ~ 201 0
10 M 85 GiP 12 25 24.053 +18 11 27.89   10.2       ~ 602 0
11 GRB 150101B gB 12 32 04.96 -10 56 00.7           ~ 85 1
12 GRB 080607 gB 12 59 47.14 +15 55 09.6           ~ 209 0
13 M 51 GiP 13 29 52.698 +47 11 42.93   9.26 8.36 8.40   ~ 3781 4
14 SN 2011dh SN* 13 30 05.10555 +47 10 10.9227           SNIIb 280 1
15 GRB 080207 gB 13 50 03.02 +07 30 08.0           ~ 87 0
16 GRB 090417B gB 13 58 44.8 +47 00 55           ~ 95 1
17 NVSS J145024-190915 Rad 14 50 24.98 -19 09 15.2           ~ 1 0
18 NVSS J145203-194308 Rad 14 52 03.58 -19 43 08.0           ~ 1 0
19 GRB 010222 gB 14 52 12.55 +43 01 06.3           ~ 335 2
20 ESO 580-49 G 14 53 07.863 -19 44 12.98   15.18   14.07   ~ 38 0
21 GRB 111005A gB 14 53 15.60 -19 43 19.1           ~ 42 0
22 ACO S 780 ClG 14 59 29.1 -18 10 45           ~ 63 0
23 GRB 080325 gB 18 31 34.40 +36 31 26.1           ~ 61 0
24 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1650 2
25 EM* MWC 349 ** 20 32 45.499080 +40 39 36.74124   15.88 13.15 12.13   Bep 707 0
26 GRB 060614 gB 21 23 32.140 -53 01 36.10 18.89 20.12 19.54     ~ 507 1
27 GRB 060505 gB 22 07 03.440 -27 48 51.89           ~ 222 1
28 GRB 020819 gB 23 00 12 -43 00.7           ~ 120 1
29 GRB 051022A gB 23 56 04.200 +19 36 32.30           ~ 163 1

    Equat.    Gal    SGal    Ecl

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2020.07.08-02:57:19

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