中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Follow Up of GW170817 and Its Electromagnetic Counterpart by Australian-Led Observing Programmes

文献类型:期刊论文

AuthorWolf, C.2,3,49; Beardsley, A.52; Andreoni, I.48,49,50; Ackley, K.47,49,51; Cooke, J.2,48,49; Acharyya, A.3,53; Allison, J. R.4,5; Anderson, G. E.6; Ashley, M. C. B.7; Baade, D.8
SourcePUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
Issued Date2017-12-20
Volume34
KeywordGamma-ray Burst: Individual: Grb170817a Gravitational Waves Stars: Neutron Supernovae: General Supernovae: Individual: At2017gfo
DOI10.1017/pasa.2017.65
SubtypeReview
English AbstractThe discovery of the first electromagnetic counterpart to a gravitational wave signal has generated follow-up observations by over 50 facilities world-wide, ushering in the new era of multi-messenger astronomy. In this paper, we present follow-up observations of the gravitational wave event GW170817 and its electromagnetic counterpart SSS17a/DLT17ck (IAU label AT2017gfo) by 14 Australian telescopes and partner observatories as part of Australian-based and Australian-led research programs. We report early- to late-time multi-wavelength observations, including optical imaging and spectroscopy, mid-infrared imaging, radio imaging, and searches for fast radio bursts. Our optical spectra reveal that the transient source emission cooled from approximately 6 400 K to 2 100 K over a 7-d period and produced no significant optical emission lines. The spectral profiles, cooling rate, and photometric light curves are consistent with the expected outburst and subsequent processes of a binary neutron star merger. Star formation in the host galaxy probably ceased at least a Gyr ago, although there is evidence for a galaxy merger. Binary pulsars with short (100 Myr) decay times are therefore unlikely progenitors, but pulsars like PSR B1534+12 with its 2.7 Gyr coalescence time could produce such a merger. The displacement (similar to 2.2 kpc) of the binary star system from the centre of the main galaxy is not unusual for stars in the host galaxy or stars originating in the merging galaxy, and therefore any constraints on the kick velocity imparted to the progenitor are poor.
WOS KeywordGAMMA-RAY BURSTS ; COMPACT OBJECT MERGERS ; ACCRETING BLACK-HOLES ; KILONOVA LIGHT CURVES ; NEUTRON-STAR MERGER ; FUNDAMENTAL PLANE ; HOST GALAXY ; RADIO-BURST ; AFTERGLOW ; TELESCOPE
WOS Research AreaAstronomy & Astrophysics
Language英语
WOS IDWOS:000418457200001
Funding OrganizationAustralian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Australian Astronomical Observatory (AAO) ; Australian Astronomical Observatory (AAO) ; Australian Research Council Future Fellowship(FT130101219) ; Australian Research Council Future Fellowship(FT130101219) ; NASA(NNX13AD28A ; NASA(NNX13AD28A ; Australian Research Council(FT150100099) ; Australian Research Council(FT150100099) ; Australian Research Council grant Laureate Fellowship(FL15010014) ; Australian Research Council grant Laureate Fellowship(FL15010014) ; NSF(AST-141242.1 PAB ; NSF(AST-141242.1 PAB ; Australian Research Council ; Australian Research Council ; Australian Government ; Australian Government ; Australian Government (NCRIS) ; Australian Government (NCRIS) ; Western Australian Government ; Western Australian Government ; National Collaborative Research Infrastructure Strategy ; National Collaborative Research Infrastructure Strategy ; Government of Western Australia ; Government of Western Australia ; Science and Industry Endowment Fund ; Science and Industry Endowment Fund ; University of Western Australia Department of Physics, in the Faculty of Engineering and Mathematical Sciences ; University of Western Australia Department of Physics, in the Faculty of Engineering and Mathematical Sciences ; ARC LIEF from the Australian Research Council(LE130100104) ; ARC LIEF from the Australian Research Council(LE130100104) ; ANU, Swinburne University of Technology ; ANU, Swinburne University of Technology ; University of Queensland ; University of Queensland ; University of Western Australia ; University of Western Australia ; University of Melbourne ; University of Melbourne ; Curtin University of Technology ; Curtin University of Technology ; Australian Astronomical Observatory ; Australian Astronomical Observatory ; National Basic Research Program (973 Program) of China(2013CB834900) ; National Basic Research Program (973 Program) of China(2013CB834900) ; Chinese Polar Environment Comprehensive Investigation&Assessment Program(CHINARE2016-02-03-05) ; Chinese Polar Environment Comprehensive Investigation&Assessment Program(CHINARE2016-02-03-05) ; Tsinghua University ; Tsinghua University ; Nanjing University ; Nanjing University ; Beijing Normal University ; Beijing Normal University ; University of New South Wales ; University of New South Wales ; Texas AM University ; Texas AM University ; Australian Antarctic Division ; Australian Antarctic Division ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; National Astronomical Observatory of China (NAOC) ; National Astronomical Observatory of China (NAOC) ; National Research Foundation (NRF) of South Africa ; National Research Foundation (NRF) of South Africa ; ESO programme(60.A-9392) ; ESO programme(60.A-9392) ; Southern African Large Telescope (SALT) under the Director's Discretionary Time programme(2017-1-DDT-009) ; Southern African Large Telescope (SALT) under the Director's Discretionary Time programme(2017-1-DDT-009) ; Monash University ; Monash University ; Australian Research Council Centre of Excellence for All-sky Astrophysics in 3 Dimensions (ASTRO-3D)(CE170100013) ; Australian Research Council Centre of Excellence for All-sky Astrophysics in 3 Dimensions (ASTRO-3D)(CE170100013) ; NNX15AP95A) ; NNX15AP95A) ; AST-1313484) ; AST-1313484) ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav)(CE170100004) ; Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO)(CE110001020) ; Australian Astronomical Observatory (AAO) ; Australian Astronomical Observatory (AAO) ; Australian Research Council Future Fellowship(FT130101219) ; Australian Research Council Future Fellowship(FT130101219) ; NASA(NNX13AD28A ; NASA(NNX13AD28A ; Australian Research Council(FT150100099) ; Australian Research Council(FT150100099) ; Australian Research Council grant Laureate Fellowship(FL15010014) ; Australian Research Council grant Laureate Fellowship(FL15010014) ; NSF(AST-141242.1 PAB ; NSF(AST-141242.1 PAB ; Australian Research Council ; Australian Research Council ; Australian Government ; Australian Government ; Australian Government (NCRIS) ; Australian Government (NCRIS) ; Western Australian Government ; Western Australian Government ; National Collaborative Research Infrastructure Strategy ; National Collaborative Research Infrastructure Strategy ; Government of Western Australia ; Government of Western Australia ; Science and Industry Endowment Fund ; Science and Industry Endowment Fund ; University of Western Australia Department of Physics, in the Faculty of Engineering and Mathematical Sciences ; University of Western Australia Department of Physics, in the Faculty of Engineering and Mathematical Sciences ; ARC LIEF from the Australian Research Council(LE130100104) ; ARC LIEF from the Australian Research Council(LE130100104) ; ANU, Swinburne University of Technology ; ANU, Swinburne University of Technology ; University of Queensland ; University of Queensland ; University of Western Australia ; University of Western Australia ; University of Melbourne ; University of Melbourne ; Curtin University of Technology ; Curtin University of Technology ; Australian Astronomical Observatory ; Australian Astronomical Observatory ; National Basic Research Program (973 Program) of China(2013CB834900) ; National Basic Research Program (973 Program) of China(2013CB834900) ; Chinese Polar Environment Comprehensive Investigation&Assessment Program(CHINARE2016-02-03-05) ; Chinese Polar Environment Comprehensive Investigation&Assessment Program(CHINARE2016-02-03-05) ; Tsinghua University ; Tsinghua University ; Nanjing University ; Nanjing University ; Beijing Normal University ; Beijing Normal University ; University of New South Wales ; University of New South Wales ; Texas AM University ; Texas AM University ; Australian Antarctic Division ; Australian Antarctic Division ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; National Collaborative Research Infrastructure Strategy (NCRIS) of Australia ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; Chinese Academy of Sciences through the Center for Astronomical Mega-Science ; National Astronomical Observatory of China (NAOC) ; National Astronomical Observatory of China (NAOC) ; National Research Foundation (NRF) of South Africa ; National Research Foundation (NRF) of South Africa ; ESO programme(60.A-9392) ; ESO programme(60.A-9392) ; Southern African Large Telescope (SALT) under the Director's Discretionary Time programme(2017-1-DDT-009) ; Southern African Large Telescope (SALT) under the Director's Discretionary Time programme(2017-1-DDT-009) ; Monash University ; Monash University ; Australian Research Council Centre of Excellence for All-sky Astrophysics in 3 Dimensions (ASTRO-3D)(CE170100013) ; Australian Research Council Centre of Excellence for All-sky Astrophysics in 3 Dimensions (ASTRO-3D)(CE170100013) ; NNX15AP95A) ; NNX15AP95A) ; AST-1313484) ; AST-1313484)
源URL[http://ir.bao.ac.cn/handle/114a11/20341]  
Collection国家天文台_星系宇宙学研究部
Affiliation1.CSIRO, ATNF, Astron & Space Sci, POB 76, Epping, NSW 1710, Australia
2.Australian Res Council, Ctr Excellence All Sky Astrophys CAASTRO, Canberra, ACT, Australia
3.Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia
4.Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia
5.Australian Res Council, Ctr Excellence All Sky Astrophys Dimens ASTRO 3D, Canberra, ACT, Australia
6.Curtin Univ, Int Ctr Radio Astron Res, Bentley, WA 6102, Australia
7.Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia
8.European Org Astron Res Southern Hemisphere ESO, Karl Schwarzschild Str 2, D-85748 Garching, Germany
9.Stockholm Univ, Dept Astron, SE-10691 Stockholm, Sweden
10.Univ Wisconsin, Dept Phys, Milwaukee, WI 53201 USA
Recommended Citation
GB/T 7714
Wolf, C.,Beardsley, A.,Andreoni, I.,et al. Follow Up of GW170817 and Its Electromagnetic Counterpart by Australian-Led Observing Programmes[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA,2017,34.
APA Wolf, C..,Beardsley, A..,Andreoni, I..,Ackley, K..,Cooke, J..,...&Zovaro, H..(2017).Follow Up of GW170817 and Its Electromagnetic Counterpart by Australian-Led Observing Programmes.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA,34.
MLA Wolf, C.,et al."Follow Up of GW170817 and Its Electromagnetic Counterpart by Australian-Led Observing Programmes".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA 34(2017).

入库方式: OAI收割

来源:国家天文台

浏览0
下载0
收藏0
其他版本

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.