脉冲星 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "脉冲星" in Chinese language version.

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13harvard.edu

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12web.archive.org

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7doi.org

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5semanticscholar.org

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3arxiv.org

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1nasa.gov

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1caltech.edu

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1nobelprize.org

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1worldcat.org

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1discovery.com

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1nrao.edu

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1esa.int

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arxiv.org

Weisberg, J.M.; Nice, D.J. & Taylor, J.H. Timing measurements of the relativistic binary pulsar PSR B1913+ 16. The Astrophysical Journal. 2010, 722 (2): 1030–1034. Bibcode:2010ApJ...722.1030W. S2CID 118573183. arXiv:1011.0718 . doi:10.1088/0004-637X/722/2/1030.
Buckley, D. A. H.; Meintjes, P. J.; Potter, S. B.; Marsh, T. R.; Gänsicke, B. T. Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii. Nature Astronomy. 2017-01-23, 1 (2): 0029. Bibcode:2017NatAs...1E..29B. ISSN 2397-3366. S2CID 15683792. arXiv:1612.03185 . doi:10.1038/s41550-016-0029 （英语）.
Angelo Tartaglia,Matteo Luca Ruggiero,Emiliano Capolongo,"A null frame for spacetime positioning by means of pulsating sources"[2] （页面存档备份，存于互联网档案馆）,arxiv.org,Oct.10th 2010.

caltech.edu

authors.library.caltech.edu

Baade, W.; Zwicky, F. Remarks on Super-Novae and Cosmic Rays (PDF). Physical Review. 1934, 46 (1): 76 [2021-03-10]. Bibcode:1934PhRv...46...76B. doi:10.1103/PhysRev.46.76.2. （原始内容存档 (PDF)于2021-02-24）.

discovery.com

news.discovery.com

Marissa Cevallos, Science News,"HOW TO USE A PULSAR TO FIND STARBUCKS"[1] （页面存档备份，存于互联网档案馆）,Discovery News,Wed Nov 24, 2010 10:21 AM ET .

doi.org

dx.doi.org

Baade, W.; Zwicky, F. Remarks on Super-Novae and Cosmic Rays (PDF). Physical Review. 1934, 46 (1): 76 [2021-03-10]. Bibcode:1934PhRv...46...76B. doi:10.1103/PhysRev.46.76.2. （原始内容存档 (PDF)于2021-02-24）.
Woltjer, L. X-rays and Type I Supernova Remnants. Astrophysical Journal. 1964, 140: 1309 [2021-03-10]. Bibcode:1964ApJ...140.1309W. doi:10.1086/148028. （原始内容存档于2020-05-10）.
Pacini, F. Energy Emission from a Neutron Star. Nature. 1967, 216 (5115): 567–568. Bibcode:1967Natur.216..567P. S2CID 4282721. doi:10.1038/216567a0.
Gold, T. Rotating Neutron Stars as the Origin of the Pulsating Radio Sources. Nature. 1968, 218 (5143): 731–732. Bibcode:1968Natur.218..731G. S2CID 4217682. doi:10.1038/218731a0.
Weisberg, J.M.; Nice, D.J. & Taylor, J.H. Timing measurements of the relativistic binary pulsar PSR B1913+ 16. The Astrophysical Journal. 2010, 722 (2): 1030–1034. Bibcode:2010ApJ...722.1030W. S2CID 118573183. arXiv:1011.0718 . doi:10.1088/0004-637X/722/2/1030.
D. Backer; Kulkarni, Shrinivas R.; Heiles, Carl; Davis, M. M.; Goss, W. M. A millisecond pulsar. Nature. 1982, 300 (5893): 315–318. Bibcode:1982Natur.300..615B. S2CID 4247734. doi:10.1038/300615a0.
Buckley, D. A. H.; Meintjes, P. J.; Potter, S. B.; Marsh, T. R.; Gänsicke, B. T. Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii. Nature Astronomy. 2017-01-23, 1 (2): 0029. Bibcode:2017NatAs...1E..29B. ISSN 2397-3366. S2CID 15683792. arXiv:1612.03185 . doi:10.1038/s41550-016-0029 （英语）.

esa.int

Old Pulsars Still Have New Tricks to Teach Us. Staff. ESA. 26 July 2006 [30 April 2013]. （原始内容存档于2012-10-19）.

harvard.edu

ui.adsabs.harvard.edu

Baade, W.; Zwicky, F. Remarks on Super-Novae and Cosmic Rays (PDF). Physical Review. 1934, 46 (1): 76 [2021-03-10]. Bibcode:1934PhRv...46...76B. doi:10.1103/PhysRev.46.76.2. （原始内容存档 (PDF)于2021-02-24）.
Woltjer, L. X-rays and Type I Supernova Remnants. Astrophysical Journal. 1964, 140: 1309 [2021-03-10]. Bibcode:1964ApJ...140.1309W. doi:10.1086/148028. （原始内容存档于2020-05-10）.
Pacini, F. Energy Emission from a Neutron Star. Nature. 1967, 216 (5115): 567–568. Bibcode:1967Natur.216..567P. S2CID 4282721. doi:10.1038/216567a0.
Gold, T. Rotating Neutron Stars as the Origin of the Pulsating Radio Sources. Nature. 1968, 218 (5143): 731–732. Bibcode:1968Natur.218..731G. S2CID 4217682. doi:10.1038/218731a0.
``Crab nebula pulsar NP 0532 （页面存档备份，存于互联网档案馆） 1969, J. M. Comella, H. D. Craft, R. V. E. Lovelace, J. M. Sutton, G. L. Tyler Nature 221 (5179), 453-454
``Digital Search Methods for Pulsars （页面存档备份，存于互联网档案馆） 1969, R. V. E. Lovelace, J. M. Sutton, E. E. Salpeter Nature 222 (5190), 231-233
Weisberg, J.M.; Nice, D.J. & Taylor, J.H. Timing measurements of the relativistic binary pulsar PSR B1913+ 16. The Astrophysical Journal. 2010, 722 (2): 1030–1034. Bibcode:2010ApJ...722.1030W. S2CID 118573183. arXiv:1011.0718 . doi:10.1088/0004-637X/722/2/1030.
D. Backer; Kulkarni, Shrinivas R.; Heiles, Carl; Davis, M. M.; Goss, W. M. A millisecond pulsar. Nature. 1982, 300 (5893): 315–318. Bibcode:1982Natur.300..615B. S2CID 4247734. doi:10.1038/300615a0.
Buckley, D. A. H.; Meintjes, P. J.; Potter, S. B.; Marsh, T. R.; Gänsicke, B. T. Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii. Nature Astronomy. 2017-01-23, 1 (2): 0029. Bibcode:2017NatAs...1E..29B. ISSN 2397-3366. S2CID 15683792. arXiv:1612.03185 . doi:10.1038/s41550-016-0029 （英语）.

adsabs.harvard.edu

An Independent 1967 Discovery of Pulsars. 40 YEARS OF PULSARS: Millisecond Pulsars, Magnetars and More. AIP Conference Proceedings, Volume 983, pp. 642-645 (2008).
Gold, T., Pacini, F., 1968, Astrophysical Journal, 152, L115. NASA ADS

articles.adsabs.harvard.edu

Woltjer, L. X-rays and Type I Supernova Remnants. Astrophysical Journal. 1964, 140: 1309 [2021-03-10]. Bibcode:1964ApJ...140.1309W. doi:10.1086/148028. （原始内容存档于2020-05-10）.
``On the discovery of the period of the Crab Nebula pulsar （页面存档备份，存于互联网档案馆） R. V. E. Lovelace and G. L. Tyler 2012, The Observatory, 132, 186.

nasa.gov

NASA's NICER Delivers Best-ever Pulsar Measurements, 1st Surface Map. [2021-03-06]. （原始内容存档于2021-03-01）.

nobelprize.org

Nobel Prize in Physics 1993. [2010-01-07]. （原始内容存档于2012-06-22）.

nrao.edu

cv.nrao.edu

Pulsars. www.cv.nrao.edu. [2021-03-10]. （原始内容存档于2020-11-12）.

nytimes.com

Sullivan, Walter. PULSAR TERMED MOST ACCURATE 'CLOCK' IN SKY. NY Times. The New York Times. February 9, 1983 [January 15, 2018]. （原始内容存档于2021-04-28）.

semanticscholar.org

api.semanticscholar.org

Pacini, F. Energy Emission from a Neutron Star. Nature. 1967, 216 (5115): 567–568. Bibcode:1967Natur.216..567P. S2CID 4282721. doi:10.1038/216567a0.
Gold, T. Rotating Neutron Stars as the Origin of the Pulsating Radio Sources. Nature. 1968, 218 (5143): 731–732. Bibcode:1968Natur.218..731G. S2CID 4217682. doi:10.1038/218731a0.
Weisberg, J.M.; Nice, D.J. & Taylor, J.H. Timing measurements of the relativistic binary pulsar PSR B1913+ 16. The Astrophysical Journal. 2010, 722 (2): 1030–1034. Bibcode:2010ApJ...722.1030W. S2CID 118573183. arXiv:1011.0718 . doi:10.1088/0004-637X/722/2/1030.
D. Backer; Kulkarni, Shrinivas R.; Heiles, Carl; Davis, M. M.; Goss, W. M. A millisecond pulsar. Nature. 1982, 300 (5893): 315–318. Bibcode:1982Natur.300..615B. S2CID 4247734. doi:10.1038/300615a0.
Buckley, D. A. H.; Meintjes, P. J.; Potter, S. B.; Marsh, T. R.; Gänsicke, B. T. Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii. Nature Astronomy. 2017-01-23, 1 (2): 0029. Bibcode:2017NatAs...1E..29B. ISSN 2397-3366. S2CID 15683792. arXiv:1612.03185 . doi:10.1038/s41550-016-0029 （英语）.

web.archive.org

秦一男. 波霎閃耀憶君山. 科學人. 2018, 200 [2023-07-26]. （原始内容存档于2023-07-26）（中文（臺灣））.
NASA's NICER Delivers Best-ever Pulsar Measurements, 1st Surface Map. [2021-03-06]. （原始内容存档于2021-03-01）.
Sullivan, Walter. PULSAR TERMED MOST ACCURATE 'CLOCK' IN SKY. NY Times. The New York Times. February 9, 1983 [January 15, 2018]. （原始内容存档于2021-04-28）.
Baade, W.; Zwicky, F. Remarks on Super-Novae and Cosmic Rays (PDF). Physical Review. 1934, 46 (1): 76 [2021-03-10]. Bibcode:1934PhRv...46...76B. doi:10.1103/PhysRev.46.76.2. （原始内容存档 (PDF)于2021-02-24）.
Woltjer, L. X-rays and Type I Supernova Remnants. Astrophysical Journal. 1964, 140: 1309 [2021-03-10]. Bibcode:1964ApJ...140.1309W. doi:10.1086/148028. （原始内容存档于2020-05-10）.
``Crab nebula pulsar NP 0532 （页面存档备份，存于互联网档案馆） 1969, J. M. Comella, H. D. Craft, R. V. E. Lovelace, J. M. Sutton, G. L. Tyler Nature 221 (5179), 453-454
``Digital Search Methods for Pulsars （页面存档备份，存于互联网档案馆） 1969, R. V. E. Lovelace, J. M. Sutton, E. E. Salpeter Nature 222 (5190), 231-233
``On the discovery of the period of the Crab Nebula pulsar （页面存档备份，存于互联网档案馆） R. V. E. Lovelace and G. L. Tyler 2012, The Observatory, 132, 186.
Marissa Cevallos, Science News,"HOW TO USE A PULSAR TO FIND STARBUCKS"[1] （页面存档备份，存于互联网档案馆）,Discovery News,Wed Nov 24, 2010 10:21 AM ET .
Angelo Tartaglia,Matteo Luca Ruggiero,Emiliano Capolongo,"A null frame for spacetime positioning by means of pulsating sources"[2] （页面存档备份，存于互联网档案馆）,arxiv.org,Oct.10th 2010.
Pulsars. www.cv.nrao.edu. [2021-03-10]. （原始内容存档于2020-11-12）.
Old Pulsars Still Have New Tricks to Teach Us. Staff. ESA. 26 July 2006 [30 April 2013]. （原始内容存档于2012-10-19）.

webcitation.org

Nobel Prize in Physics 1993. [2010-01-07]. （原始内容存档于2012-06-22）.

worldcat.org

Buckley, D. A. H.; Meintjes, P. J.; Potter, S. B.; Marsh, T. R.; Gänsicke, B. T. Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii. Nature Astronomy. 2017-01-23, 1 (2): 0029. Bibcode:2017NatAs...1E..29B. ISSN 2397-3366. S2CID 15683792. arXiv:1612.03185 . doi:10.1038/s41550-016-0029 （英语）.

ylib.com

sa.ylib.com

秦一男. 波霎閃耀憶君山. 科學人. 2018, 200 [2023-07-26]. （原始内容存档于2023-07-26）（中文（臺灣））.