中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
首页 机构 成果 学者
  
  1. CAS IR Grid
  2. 国家天文台
  3. 中国科学院国家天文台
PSR J2234+0611: A New Laboratory for Stellar Evolution

文献类型：期刊论文

作者Stovall, K.1; Freire, P. C. C.2; Antoniadis, J.2; Bagchi, M.3; Deneva, J. S.4; Garver-Daniels, N.5,6; Martinez, J. G.2; McLaughlin, M. A.5,6; Arzoumanian, Z.7,8; Blumer, H.5,6
刊名ASTROPHYSICAL JOURNAL
出版日期2019-01-10
卷号870期号:2页码:13
关键词pulsars: individual (PSR J2234+0611) white dwarfs
ISSN号0004-637X
DOI10.3847/1538-4357/aaf37d
英文摘要We report the timing results for PSR J2234+0611, a 3.6 ms pulsar in a 32 day, eccentric (e = 0.13) orbit with a helium white dwarf. The precise timing and eccentric nature of the orbit allow measurements of an unusual number of parameters: (a) a precise proper motion of 27.10(3) mas yr(-1) and a parallax of 1.05(4) mas resulting in a pulsar distance of 0.95(4) kpc; enabling an estimate of the transverse velocity, 123(5) km s(-1). Together with previously published spectroscopic measurements of the systemic radial velocity, this allows a 3D determination of the system's velocity; (b) precise measurements of the rate of advance of periastron yields a total system mass of 1.6518(-0.0035)(+0.0033) M-circle dot; (c) a Shapiro delay measurement, h(3) = 82 +/- 14 ns, despite the orbital inclination not being near 90 degrees; combined with the measurement of the total mass yields a pulsar mass of 1.353(-0.017)(+0.014) M-circle dot and a companion mass of 0.298(-0.012)(+0.015) M-circle dot; (d) we measure precisely the secular variation of the projected semimajor axis and detect a significant annual orbital parallax; together these allow a determination of the 3D orbital geometry of the system, including an unambiguous orbital inclination (i = 138.7(-2.2)(+2.5) deg) and a position angle for the line of nodes (Omega = 44(-4)(+5) deg). We discuss the component masses to investigate the hypotheses previously advanced to explain the origin of eccentric MSPs. The unprecedented determination of the 3D position, motion, and orbital orientation of the system, plus the precise pulsar and WD masses and the latter's optical detection make this system a unique test of our understanding of white dwarfs and their atmospheres.
WOS关键词RELATIVISTIC CELESTIAL MECHANICS ; BINARY MILLISECOND PULSAR ; GENERAL-RELATIVITY ; MASSES ; SYSTEMS
资助项目National Science Foundation (NSF)[AST-1744119] ; NANOGrav Physics Frontiers Center (NSF)[1430284] ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013)[279702] ; Max Planck Society ; NASA Fermi program ; NSERC Discovery Grant ; Canadian Institute for Advanced Research ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000455820100020
出版者IOP PUBLISHING LTD
资助机构National Science Foundation (NSF) ; National Science Foundation (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; Max Planck Society ; Max Planck Society ; NASA Fermi program ; NASA Fermi program ; NSERC Discovery Grant ; NSERC Discovery Grant ; Canadian Institute for Advanced Research ; Canadian Institute for Advanced Research ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; Max Planck Society ; Max Planck Society ; NASA Fermi program ; NASA Fermi program ; NSERC Discovery Grant ; NSERC Discovery Grant ; Canadian Institute for Advanced Research ; Canadian Institute for Advanced Research ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; Max Planck Society ; Max Planck Society ; NASA Fermi program ; NASA Fermi program ; NSERC Discovery Grant ; NSERC Discovery Grant ; Canadian Institute for Advanced Research ; Canadian Institute for Advanced Research ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; National Science Foundation (NSF) ; National Science Foundation (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; NANOGrav Physics Frontiers Center (NSF) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; European Research Council, under the European Union's Seventh Framework Programme (FP/2007-2013) ; Max Planck Society ; Max Planck Society ; NASA Fermi program ; NASA Fermi program ; NSERC Discovery Grant ; NSERC Discovery Grant ; Canadian Institute for Advanced Research ; Canadian Institute for Advanced Research ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne ; International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne
源URL[http://ir.bao.ac.cn/handle/114a11/24655]  
专题中国科学院国家天文台
通讯作者Stovall, K.
作者单位1.Natl Radio Astron Observ, 1003 Lopezville Rd, Socorro, NM 87801 USA
2.Max Planck Inst Radioastron, Auf Dem Hugel 69, D-53131 Bonn, Germany
3.Inst Math Sci, Madras 600113, Tamil Nadu, India
4.George Mason Univ, Naval Res Lab, 4555 Overlook Ave SW, Washington, DC 20375 USA
5.West Virginia Univ, Dept Phys & Astron, POB 6315, Morgantown, WV 26506 USA
6.West Virginia Univ, Ctr Gravitat Waves & Cosmol, Chestnut Ridge Res Bldg, Morgantown, WV 26505 USA
7.NASA, Goddard Space Flight Ctr, Ctr Res & Explorat Space Sci & Technol, Code 662, Greenbelt, MD 20771 USA
8.NASA, Goddard Space Flight Ctr, Xray Astrophys Lab, Code 662, Greenbelt, MD 20771 USA
9.Univ Virginia, Dept Astron, POB 400325, Charlottesville, VA 22904 USA
10.Lafayette Coll, Dept Phys, Easton, PA 18042 USA
推荐引用方式
GB/T 7714		 Stovall, K.,Freire, P. C. C.,Antoniadis, J.,et al. PSR J2234+0611: A New Laboratory for Stellar Evolution[J]. ASTROPHYSICAL JOURNAL,2019,870(2):13.
APA Stovall, K..,Freire, P. C. C..,Antoniadis, J..,Bagchi, M..,Deneva, J. S..,...&Zhu, W. W..(2019).PSR J2234+0611: A New Laboratory for Stellar Evolution.ASTROPHYSICAL JOURNAL,870(2),13.
MLA Stovall, K.,et al."PSR J2234+0611: A New Laboratory for Stellar Evolution".ASTROPHYSICAL JOURNAL 870.2(2019):13.

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

除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。