中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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
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
DOI10.1093/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
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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.

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