White dwarf-main sequence binaries from LAMOST: the DR5 catalogue
文献类型:期刊论文
作者 | Ren, J. -J.1; Rebassa-Mansergas, A.2,3; Parsons, S. G.4; Liu, X. -W.5; Luo, A. -L.1; Kong, X.1,6; Zhang, H. -T.1 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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出版日期 | 2018-07-01 |
卷号 | 477期号:4页码:4641-4654 |
关键词 | binaries: close binaries: spectroscopic stars: low-mass white dwarfs |
ISSN号 | 0035-8711 |
DOI | 10.1093/mnras/sty805 |
英文摘要 | We present the data release (DR) 5 catalogue of white dwarf-main sequence (WDMS) binaries from the Large sky Area Multi-Object fibre Spectroscopic Telescope (LAMOST). The catalogue contains 876 WDMS binaries, of which 757 are additions to our previous LAMOST DR1 sample and 357 are systems that have not been published before. We also describe a LAMOST dedicated survey that aims at obtaining spectra of photometrically selected WDMS binaries from the Sloan Digital Sky Survey (SDSS) that are expected to contain cool white dwarfs and/or early-type M dwarf companions. This is a population under-represented in previous SDSS WDMS binary catalogues. We determine the stellar parameters (white dwarf effective temperatures, surface gravities and masses, and M dwarf spectral types) of the LAMOST DR5 WDMS binaries and make use of the parameter distributions to analyse the properties of the sample. We find that, despite our efforts, systems containing cool white dwarfs remain under-represented. Moreover, we make use of LAMOST DR5 and SDSS DR14 (when available) spectra to measure the Na I lambda lambda 8183.27, 8194.81 absorption doublet and/or Ha emission radial velocities of our systems. This allows identifying 128 binaries displaying significant radial velocity variations, 76 of which are new. Finally, we cross-match our catalogue with the Catalina Surveys and identify 57 systems displaying light-curve variations. These include 16 eclipsing systems, two of which are new, and nine binaries that are new eclipsing candidates. We calculate periodograms from the photometric data and measure (estimate) the orbital periods of 30 (15) WDMS binaries. |
WOS关键词 | COMMON-ENVELOPE BINARIES ; DIGITAL-SKY-SURVEY ; SUBDWARF-B-STARS ; IA SUPERNOVAE ; DATA RELEASE ; ORBITAL PERIOD ; CATACLYSMIC VARIABLES ; SPECTROSCOPIC SURVEY ; SPECTRAL-ANALYSIS ; ECLIPSING BINARY |
资助项目 | National Natural Science Foundation of China[U1531244] ; National Key Basic Research Program of China[2014CB845700] ; Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences ; MINECO under the Ramon y Cajal programme[RYC-2016-20254] ; AGAUR[SGR-661/2017] ; National Development and Reform Commission ; [AYA2017-86274-P] |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:000435630100027 |
出版者 | OXFORD UNIV PRESS |
资助机构 | National Natural Science Foundation of China ; National Key Basic Research Program of China ; Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences ; MINECO under the Ramon y Cajal programme ; AGAUR ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Key Basic Research Program of China ; Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences ; MINECO under the Ramon y Cajal programme ; AGAUR ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Key Basic Research Program of China ; Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences ; MINECO under the Ramon y Cajal programme ; AGAUR ; National Development and Reform Commission ; National Natural Science Foundation of China ; National Key Basic Research Program of China ; Young Researcher Grant of National Astronomical Observatories, Chinese Academy of Sciences ; MINECO under the Ramon y Cajal programme ; AGAUR ; National Development and Reform Commission |
源URL | [http://ir.bao.ac.cn/handle/114a11/21957] ![]() |
专题 | 中国科学院国家天文台 |
通讯作者 | Ren, J. -J. |
作者单位 | 1.Chinese Acad Sci, Key Lab Opt Astron, Natl Astron Observ, Beijing 100012, Peoples R China 2.Univ Politecn Cataluna, Dept Fis, C Esteve Terrades 5, E-08860 Castelldefels, Spain 3.Inst Space Studies Catalonia, C Gran Capita 2-4,Edif Nexus 201, E-08034 Barcelona, Spain 4.Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England 5.Yunnan Univ, South Western Inst Astron Res, Kunming 650091, Yunnan, Peoples R China 6.Univ Chinese Acad Sci, Beijing 10049, Peoples R China |
推荐引用方式 GB/T 7714 | Ren, J. -J.,Rebassa-Mansergas, A.,Parsons, S. G.,et al. White dwarf-main sequence binaries from LAMOST: the DR5 catalogue[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,477(4):4641-4654. |
APA | Ren, J. -J..,Rebassa-Mansergas, A..,Parsons, S. G..,Liu, X. -W..,Luo, A. -L..,...&Zhang, H. -T..(2018).White dwarf-main sequence binaries from LAMOST: the DR5 catalogue.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,477(4),4641-4654. |
MLA | Ren, J. -J.,et al."White dwarf-main sequence binaries from LAMOST: the DR5 catalogue".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 477.4(2018):4641-4654. |
入库方式: OAI收割
来源:国家天文台
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