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

文献类型：期刊论文

作者Michalowski, Michal J.2,3; Xu, Dong4,5; Stevens, Jamie6; Levan, Andrew7; Yang, Jun8,9; Paragi, Zsolt9; Kamble, Atish10; Tsai, An-Li2; Dannerbauer, Helmut1,11,12; van der Horst, Alexander J.13
刊名ASTRONOMY & ASTROPHYSICS
出版日期2018-09-11
卷号616页码:15
ISSN号1432-0746
关键词dust, extinction galaxies: abundances galaxies: individual: ESO 580-49 galaxies: star formation gamma-ray burst: general gamma-ray burst: individual: 111005A
DOI10.1051/0004-6361/201629942
英文摘要We report the detection of the radio afterglow of a long gamma-ray burst (GRB) 111005A at 5-345 GHz, 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 (similar to 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 similar to 20 times fainter than other SNe associated with GRBs. Moreover, we measured a twice-solar metallicity for the GRB location. The low gamma-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.
WOS关键词SCUBA SUBMILLIMETER OBSERVATIONS ; GALAXY-EVOLUTION-EXPLORER ; 25 APRIL 1998 ; HOST GALAXY ; STAR-FORMATION ; MOLECULAR GAS ; SKY SURVEY ; 980425/SN 1998BW ; RADIO AFTERGLOW ; NEARBY GALAXIES
资助项目National Science Centre, Poland through the POLONEZ grant[2015/19/P/ST9/04010] ; UK Science and Technology Facilities Council ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; European Union[665778] ; European Union[RI-261525 NEXPReS] ; Danish National Research Foundation ; Spanish Ministry of Economy and Competitiveness (MINECO)[MINECO RYC-2014-15686] ; National Basic Research Program of China[2014CB845800] ; National Natural Science Foundation of China[11361140349] ; National Natural Science Foundation of China[11103083] ; Commonwealth of Australia ; EVN project[RP018] ; European Commission[227290] ; INSU/CNRS (France) ; MPG (Germany) ; IGN (Spain) ; Netherlands Foundation for Scientific Research (NWO) ; ESO Telescopes at the La Silla Paranal Observatory[288.D-5004] ; ESO Telescopes at the La Silla Paranal Observatory[088.D-0523] ; ESO Telescopes at the La Silla Paranal Observatory[090.A-0088] ; NASA[NAS 5-26555] ; NASA[13949] ; National Aeronautics and Space Administration ; National Science Foundation ; Robert Martin Ayers Sciences Fund ; Spitzer/NASA grant RSA Agreement[1287913]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者EDP SCIENCES S A
WOS记录号WOS:000444245000001
资助机构National Science Centre, Poland through the POLONEZ grant ; National Science Centre, Poland through the POLONEZ grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; European Union ; European Union ; Danish National Research Foundation ; Danish National Research Foundation ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; National Basic Research Program of China ; National Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Commonwealth of Australia ; Commonwealth of Australia ; EVN project ; EVN project ; European Commission ; European Commission ; INSU/CNRS (France) ; INSU/CNRS (France) ; MPG (Germany) ; MPG (Germany) ; IGN (Spain) ; IGN (Spain) ; Netherlands Foundation for Scientific Research (NWO) ; Netherlands Foundation for Scientific Research (NWO) ; ESO Telescopes at the La Silla Paranal Observatory ; ESO Telescopes at the La Silla Paranal Observatory ; NASA ; NASA ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Spitzer/NASA grant RSA Agreement ; Spitzer/NASA grant RSA Agreement ; National Science Centre, Poland through the POLONEZ grant ; National Science Centre, Poland through the POLONEZ grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; European Union ; European Union ; Danish National Research Foundation ; Danish National Research Foundation ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; National Basic Research Program of China ; National Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Commonwealth of Australia ; Commonwealth of Australia ; EVN project ; EVN project ; European Commission ; European Commission ; INSU/CNRS (France) ; INSU/CNRS (France) ; MPG (Germany) ; MPG (Germany) ; IGN (Spain) ; IGN (Spain) ; Netherlands Foundation for Scientific Research (NWO) ; Netherlands Foundation for Scientific Research (NWO) ; ESO Telescopes at the La Silla Paranal Observatory ; ESO Telescopes at the La Silla Paranal Observatory ; NASA ; NASA ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Spitzer/NASA grant RSA Agreement ; Spitzer/NASA grant RSA Agreement ; National Science Centre, Poland through the POLONEZ grant ; National Science Centre, Poland through the POLONEZ grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; European Union ; European Union ; Danish National Research Foundation ; Danish National Research Foundation ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; National Basic Research Program of China ; National Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Commonwealth of Australia ; Commonwealth of Australia ; EVN project ; EVN project ; European Commission ; European Commission ; INSU/CNRS (France) ; INSU/CNRS (France) ; MPG (Germany) ; MPG (Germany) ; IGN (Spain) ; IGN (Spain) ; Netherlands Foundation for Scientific Research (NWO) ; Netherlands Foundation for Scientific Research (NWO) ; ESO Telescopes at the La Silla Paranal Observatory ; ESO Telescopes at the La Silla Paranal Observatory ; NASA ; NASA ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Spitzer/NASA grant RSA Agreement ; Spitzer/NASA grant RSA Agreement ; National Science Centre, Poland through the POLONEZ grant ; National Science Centre, Poland through the POLONEZ grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; SUPA Postdoctoral and Early Career Researcher Exchange Program ; European Union ; European Union ; Danish National Research Foundation ; Danish National Research Foundation ; Spanish Ministry of Economy and Competitiveness (MINECO) ; Spanish Ministry of Economy and Competitiveness (MINECO) ; National Basic Research Program of China ; National Basic Research Program of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Commonwealth of Australia ; Commonwealth of Australia ; EVN project ; EVN project ; European Commission ; European Commission ; INSU/CNRS (France) ; INSU/CNRS (France) ; MPG (Germany) ; MPG (Germany) ; IGN (Spain) ; IGN (Spain) ; Netherlands Foundation for Scientific Research (NWO) ; Netherlands Foundation for Scientific Research (NWO) ; ESO Telescopes at the La Silla Paranal Observatory ; ESO Telescopes at the La Silla Paranal Observatory ; NASA ; NASA ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; National Science Foundation ; National Science Foundation ; Robert Martin Ayers Sciences Fund ; Robert Martin Ayers Sciences Fund ; Spitzer/NASA grant RSA Agreement ; Spitzer/NASA grant RSA Agreement
源URL[http://ir.bao.ac.cn/handle/114a11/23167]  
专题中国科学院国家天文台
通讯作者Michalowski, Michal J.
作者单位1.Inst Astrofis Canarias, Tenerife 38205, Spain
2.Adam Mickiewicz Univ, Fac Phys, Astron Observ Inst, Ul Sloneczna 36, PL-60286 Poznan, Poland
3.Univ Edinburgh, Royal Observ, Inst Astron, SUPA, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
4.Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, Juliane Manes Vej 30, DK-2100 Copenhagen O, Denmark
5.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
6.CSIRO Astron & Space Sci, Locked Bag 194, Narrabri, NSW 2390, Australia
7.Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England
8.Chalmers Univ Technol, Onsala Space Observ, Dept Earth & Space Sci, S-43992 Onsala, Sweden
9.Joint Inst VLBI ERIC, Postbus 2, NL-7990 AA Dwingeloo, Netherlands
10.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
推荐引用方式
GB/T 7714		 Michalowski, Michal J.,Xu, Dong,Stevens, Jamie,et al. The second-closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environment[J]. ASTRONOMY & ASTROPHYSICS,2018,616:15.
APA Michalowski, Michal J..,Xu, Dong.,Stevens, Jamie.,Levan, Andrew.,Yang, Jun.,...&Bartczak, Przemyslaw.(2018).The second-closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environment.ASTRONOMY & ASTROPHYSICS,616,15.
MLA Michalowski, Michal J.,et al."The second-closest gamma-ray burst: sub-luminous GRB 111005A with no supernova in a super-solar metallicity environment".ASTRONOMY & ASTROPHYSICS 616(2018):15.

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