NAOC Open IR
Common envelope episodes that lead to double neutron star formation
Vigna-Gomez, Alejandro1,2,3,4,5; MacLeod, Morgan6; Neijssel, Coenraad J.2,3,4,5; Broekgaarden, Floor S.4,5,6; Justham, Stephen7,8,9; Howitt, George4,10; de Mink, Selma E.6,9; Vinciguerra, Serena3,4,5,11; Mandel, Ilya2,3,4,5
2020
Source PublicationPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
ISSN1323-3580
Volume37Pages:19
AbstractClose double neutron stars (DNSs) have been observed as Galactic radio pulsars, while their mergers have been detected as gamma-ray bursts and gravitational wave sources. They are believed to have experienced at least one common envelope episode (CEE) during their evolution prior to DNS formation. In the last decades, there have been numerous efforts to understand the details of the common envelope (CE) phase, but its computational modelling remains challenging. We present and discuss the properties of the donor and the binary at the onset of the Roche lobe overflow (RLOF) leading to these CEEs as predicted by rapid binary population synthesis models. These properties can be used as initial conditions for detailed simulations of the CE phase. There are three distinctive populations, classified by the evolutionary stage of the donor at the moment of the onset of the RLOF: giant donors with fully convective envelopes, cool donors with partially convective envelopes, and hot donors with radiative envelopes. We also estimate that, for standard assumptions, tides would not circularise a large fraction of these systems by the onset of RLOF. This makes the study and understanding of eccentric mass-transferring systems relevant for DNS populations.
Keywordbinaries common envelope mass transfer neutron stars population synthesis
Funding OrganizationConsejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council
DOI10.1017/pasa.2020.31
WOS KeywordCONSERVATIVE MASS-TRANSFER ; SECULAR ORBITAL EVOLUTION ; TIDAL CAPTURE BINARIES ; X-RAY ; INTERACTING BINARIES ; BLACK-HOLE ; POPULATION SYNTHESIS ; ECCENTRIC BINARIES ; STELLAR EVOLUTION ; DYNAMICAL TIDES
Language英语
Funding ProjectConsejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation[DNRF132] ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center[PF6-170169] ; NASA[NAS8-03060] ; National Science Foundation[1909203] ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves[639.042.728] ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC)[715063] ; Australian Research Council[FT190100574]
Funding OrganizationConsejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Consejo Nacional de Ciencia y Tecnologia (CONACYT) ; Danish National Research Foundation ; Danish National Research Foundation ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA through Einstein Postdoctoral Fellowship - Chandra X-ray Center ; NASA ; NASA ; National Science Foundation ; National Science Foundation ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; Netherlands Organization for Scientific Research (NWO) as part of the Vidi research programme BinWaves ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; European Union's Horizon 2020 research and innovation programme from the European Research Council (ERC) ; Australian Research Council ; Australian Research Council
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000572115400001
PublisherCAMBRIDGE UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/81404
Collection中国科学院国家天文台
Corresponding AuthorVigna-Gomez, Alejandro
Affiliation1.Univ Copenhagen, Niels Bohr Inst, DARK, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
2.Univ Birmingham, Birmingham Inst Gravitat Wave Astron, Birmingham B15 2TT, W Midlands, England
3.Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England
4.Monash Univ, Sch Phys & Astron, Monash Ctr Astrophys, Clayton, Vic 3800, Australia
5.ARC Ctr Excellence Gravitat Wave Discovery OzGrav, Hawthorn, Vic, Australia
6.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA USA
7.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100012, Peoples R China
8.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
9.Univ Amsterdam, Anton Pannekoek Inst Astron, Postbus 94249, NL-1090 GE Amsterdam, Netherlands
10.Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia
11.Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-30167 Hannover, Germany
Recommended Citation
GB/T 7714
Vigna-Gomez, Alejandro,MacLeod, Morgan,Neijssel, Coenraad J.,et al. Common envelope episodes that lead to double neutron star formation[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA,2020,37:19.
APA Vigna-Gomez, Alejandro.,MacLeod, Morgan.,Neijssel, Coenraad J..,Broekgaarden, Floor S..,Justham, Stephen.,...&Mandel, Ilya.(2020).Common envelope episodes that lead to double neutron star formation.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA,37,19.
MLA Vigna-Gomez, Alejandro,et al."Common envelope episodes that lead to double neutron star formation".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA 37(2020):19.
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