The white dwarf binary pathways survey - II. Radial velocities of 1453 FGK stars with white dwarf companions from LAMOST DR4
文献类型:期刊论文
作者 | Rebassa-Mansergas, A.1,2; Ren, J. J.3; Irawati, P.4; Garcia-Berro, E.1,2; Parsons, S. G.5; Schreiber, M. R.6; Gansicke, B. T.7; Rodriguez-Gil, P.8,9; Liu, X.10; Manser, C.7 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
出版日期 | 2017-12-01 |
卷号 | 472期号:4页码:4193-4203 |
ISSN号 | 0035-8711 |
关键词 | Stars: Low-mass White Dwarfs Binaries (Including Multiple): Close |
DOI | 10.1093/mnras/stx2259 |
产权排序 | 第13完成单位 |
文献子类 | Article |
英文摘要 | We present the second paper of a series of publications aiming at obtaining a better understanding regarding the nature of type Ia supernovae (SN Ia) progenitors by studying a large sample of detached F, G and K main-sequence stars in close orbits with white dwarf companions (i.e. WD+FGK binaries). We employ the Large Sky Area Multi-Object Fibre Spectroscopic Telescope (LAMOST) data release 4 spectroscopic data base together with Galaxy Evolution Explorer (GALEX) ultraviolet fluxes to identify 1549 WD+FGK binary candidates (1057 of which are new), thus doubling the number of known sources. We measure the radial velocities of 1453 of these binaries from the available LAMOST spectra and/or from spectra obtained by us at a wide variety of different telescopes around the globe. The analysis of the radial velocity data allows us to identify 24 systems displaying more than 3s radial velocity variation that we classify as close binaries. We also discuss the fraction of close binaries among WD+FGK systems, which we find to be similar to 10 per cent, and demonstrate that high-resolution spectroscopy is required to efficiently identify double-degenerate SN Ia progenitor candidates. |
学科主题 | 天文学 ; 恒星与银河系 |
URL标识 | 查看原文 |
出版地 | GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND |
WOS关键词 | COMMON-ENVELOPE BINARIES ; DELAY-TIME DISTRIBUTION ; CORE-DEGENERATE SCENARIO ; MAIN-SEQUENCE BINARIES ; NEBULA HENIZE 2-428 ; IA SUPERNOVAE ; CATACLYSMIC VARIABLES ; OBSERVATIONAL EVIDENCE ; ABSOLUTE MAGNITUDES ; ORBITAL PERIOD |
资助项目 | Agencia de Gestio d'Ajuts Universitaris i de Recerca ; Agencia de Gestio d'Ajuts Universitaris i de Recerca[AYA2014-59084-P] ; Agencia de Gestio d'Ajuts Universitaris i de Recerca[AYA2014-55840-P] ; Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences ; Key Basic Research Program of China[2014CB845700] ; Leverhulme Trust ; European Research Council under the European Union's Seventh Framework Programme (FP)/ERC grant[320964] ; Fondecyt[1141269] ; National Development and Reform Commission ; Palomar Hale Telescope (through Chinese Telescope Access Program)[2013B-20] ; Isaac Newton Telescope (programs)[2014B-80] ; Isaac Newton Telescope (programs)[2015B-7] ; Isaac Newton Telescope (programs)[2016B-33] ; Canada France Hawaii Telescope (through Chinese Telescope Access Program)[2015B-27] ; Telescopio Nazionale Galileo (program)[CAT17A-5] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | OXFORD UNIV PRESS |
WOS记录号 | WOS:000415652500033 |
资助机构 | Agencia de Gestio d'Ajuts Universitaris i de Recerca ; Agencia de Gestio d'Ajuts Universitaris i de Recerca[AYA2014-59084-P, AYA2014-55840-P] ; Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences ; Key Basic Research Program of China[2014CB845700] ; Leverhulme Trust ; European Research Council under the European Union's Seventh Framework Programme (FP)/ERC grant[320964] ; Fondecyt[1141269] ; National Development and Reform Commission ; Palomar Hale Telescope (through Chinese Telescope Access Program)[2013B-20] ; Isaac Newton Telescope (programs)[2014B-80, 2015B-7, 2016B-33] ; Canada France Hawaii Telescope (through Chinese Telescope Access Program)[2015B-27] ; Telescopio Nazionale Galileo (program)[CAT17A-5] |
源URL | [http://ir.ynao.ac.cn/handle/114a53/12192] |
专题 | 云南天文台_大样本恒星演化研究组 云南天文台_中国科学院天体结构与演化重点实验室 |
通讯作者 | Rebassa-Mansergas, A. |
作者单位 | 1.Departament de F´ısica, Universitat Politecnica de Catalunya, c/Esteve Terrades 5, E-08860 Castelldefels, Spain 2.Institute for Space Studies of Catalonia, c/Gran Capita 2–4, Edif. Nexus 201, E-08034 Barcelona, Spain 3.National Astronomical Observatories, Chinese Academy of Sciences, 100012 Beijing, P. R. China 4.National Astronomical Research Institute of Thailand, Sirindhorn AstroPark, Donkaew, Mae Rim, Chiang Mai 50180, Thailand 5.Deparment of Physics & Astronomy, University of Sheffield, Sheffield S3 7RH, UK 6.Instituto de F´ısica y Astronom´ıa, Universidad de Valpara´ıso, Avenida Gran Bretana 1111, Valpara ˜ ´ıso, Chile 7.Department of Physics, University of Warwick, Coventry CV4 7AL, UK 8.Instituto de Astrof´ısica de Canarias, c/ V´ıa Lactea s/n, E-38205 La Laguna, Tenerife, Spain 9.Universidad de La Laguna, Departamento de Astrof´ısica, E-38206 La Laguna, Tenerife, Spain 10.Department of Astronomy, Peking University, Beijing 100871, P. R. China |
推荐引用方式 GB/T 7714 | Rebassa-Mansergas, A.,Ren, J. J.,Irawati, P.,et al. The white dwarf binary pathways survey - II. Radial velocities of 1453 FGK stars with white dwarf companions from LAMOST DR4[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,472(4):4193-4203. |
APA | Rebassa-Mansergas, A..,Ren, J. J..,Irawati, P..,Garcia-Berro, E..,Parsons, S. G..,...&Kong, X..(2017).The white dwarf binary pathways survey - II. Radial velocities of 1453 FGK stars with white dwarf companions from LAMOST DR4.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,472(4),4193-4203. |
MLA | Rebassa-Mansergas, A.,et al."The white dwarf binary pathways survey - II. Radial velocities of 1453 FGK stars with white dwarf companions from LAMOST DR4".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 472.4(2017):4193-4203. |
入库方式: OAI收割
来源:云南天文台
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