PSR J0348+0432 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "PSR J0348+0432" in Chinese language version.

refsWebsite

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7web.archive.org

1^st place

5nature.com

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4harvard.edu

18^th place

57^th place

1sciencemag.org

857^th place

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1iop.org

1,725^th place

1,164^th place

1nih.gov

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1mpg.de

1,624^th place

1,637^th place

harvard.edu

adsabs.harvard.edu

Demorest et al. (2010) Demorest, P. B.; Pennucci, T.; Ransom, S. M.; Roberts, M. S. E.; Hessels, J. W. T. (2010). "A two-solar-mass neutron star measured using Shapiro delay". Nature 467 (7319): 1081–1083. Bibcode:2010Natur.467.1081D（页面存档备份，存于互联网档案馆）. doi:10.1038/nature09466（页面存档备份，存于互联网档案馆）. PMID 20981094（页面存档备份，存于互联网档案馆）
Hewish et al. (1968) Hewish, A.; Bell, S. J.; Pilkington, J. D. H.; Scott, P. F.; Collins, R. A. (1968). "Observation of a Rapidly Pulsating Radio Source". Nature 217 (5130): 709. Bibcode:1968Natur.217..709H（页面存档备份，存于互联网档案馆）. doi:10.1038/217709a0（页面存档备份，存于互联网档案馆）.
Pacini (1968) Pacini, F. (1968). "Rotating Neutron Stars, Pulsars and Supernova Remnants". Nature 219 (5150): 145. Bibcode:1968Natur.219..145P（页面存档备份，存于互联网档案馆）. doi:10.1038/219145a0.
Gold (1968) Gold, T. (1968). "Rotating Neutron Stars as the Origin of the Pulsating Radio Sources". Nature 218 (5143): 731. Bibcode:1968Natur.218..731G（页面存档备份，存于互联网档案馆）. doi:10.1038/218731a0（页面存档备份，存于互联网档案馆）.

iop.org

iopscience.iop.org

Lynch et al. (2013) Lynch, R. S.; Boyles, J.; Ransom, S. M.; Stairs, I. H.; Lorimer, D. R.; McLaughlin, M. A.; Hessels, J. W. T.; Kaspi, V. M. et al. (2013). "THE GREEN BANK TELESCOPE 350 MHz DRIFT-SCAN SURVEY II: DATA ANALYSIS AND THE TIMING OF 10 NEW PULSARS, INCLUDING a RELATIVISTIC BINARY". The Astrophysical Journal 763 (2): 81. doi:10.1088/0004-637X/763/2/81.

mpg.de

A heavyweight for Einstein. Max Planck Institute for Radio Astronomy, Bonn. 25 April 2013 [13 May 2013]. （原始内容存档于2013-06-24）.

nature.com

Demorest et al. (2010) Demorest, P. B.; Pennucci, T.; Ransom, S. M.; Roberts, M. S. E.; Hessels, J. W. T. (2010). "A two-solar-mass neutron star measured using Shapiro delay". Nature 467 (7319): 1081–1083. Bibcode:2010Natur.467.1081D（页面存档备份，存于互联网档案馆）. doi:10.1038/nature09466（页面存档备份，存于互联网档案馆）. PMID 20981094（页面存档备份，存于互联网档案馆）
Hewish et al. (1968) Hewish, A.; Bell, S. J.; Pilkington, J. D. H.; Scott, P. F.; Collins, R. A. (1968). "Observation of a Rapidly Pulsating Radio Source". Nature 217 (5130): 709. Bibcode:1968Natur.217..709H（页面存档备份，存于互联网档案馆）. doi:10.1038/217709a0（页面存档备份，存于互联网档案馆）.
Pacini (1968) Pacini, F. (1968). "Rotating Neutron Stars, Pulsars and Supernova Remnants". Nature 219 (5150): 145. Bibcode:1968Natur.219..145P（页面存档备份，存于互联网档案馆）. doi:10.1038/219145a0.
Gold (1968) Gold, T. (1968). "Rotating Neutron Stars as the Origin of the Pulsating Radio Sources". Nature 218 (5143): 731. Bibcode:1968Natur.218..731G（页面存档备份，存于互联网档案馆）. doi:10.1038/218731a0（页面存档备份，存于互联网档案馆）.
Massive double star is latest test for Einstein’s gravity theory. Ron Cowen. Nature. 25 April 2013 [12 May 2013]. （原始内容存档于2013-06-01）.

nih.gov

ncbi.nlm.nih.gov

Demorest et al. (2010) Demorest, P. B.; Pennucci, T.; Ransom, S. M.; Roberts, M. S. E.; Hessels, J. W. T. (2010). "A two-solar-mass neutron star measured using Shapiro delay". Nature 467 (7319): 1081–1083. Bibcode:2010Natur.467.1081D（页面存档备份，存于互联网档案馆）. doi:10.1038/nature09466（页面存档备份，存于互联网档案馆）. PMID 20981094（页面存档备份，存于互联网档案馆）

sciencemag.org

Antoniadis et al. (2013) Antoniadis, J.; Freire, P. C. C.; Wex, N.; Tauris, T. M.; Lynch, R. S.; Van Kerkwijk, M. H.; Kramer, M.; Bassa, C. et al. (2013). "A Massive Pulsar in a Compact Relativistic Binary". Science 340 (6131): 1233232. doi:10.1126/science.1233232（页面存档备份，存于互联网档案馆）.

web.archive.org

Antoniadis et al. (2013) Antoniadis, J.; Freire, P. C. C.; Wex, N.; Tauris, T. M.; Lynch, R. S.; Van Kerkwijk, M. H.; Kramer, M.; Bassa, C. et al. (2013). "A Massive Pulsar in a Compact Relativistic Binary". Science 340 (6131): 1233232. doi:10.1126/science.1233232（页面存档备份，存于互联网档案馆）.
Demorest et al. (2010) Demorest, P. B.; Pennucci, T.; Ransom, S. M.; Roberts, M. S. E.; Hessels, J. W. T. (2010). "A two-solar-mass neutron star measured using Shapiro delay". Nature 467 (7319): 1081–1083. Bibcode:2010Natur.467.1081D（页面存档备份，存于互联网档案馆）. doi:10.1038/nature09466（页面存档备份，存于互联网档案馆）. PMID 20981094（页面存档备份，存于互联网档案馆）
Hewish et al. (1968) Hewish, A.; Bell, S. J.; Pilkington, J. D. H.; Scott, P. F.; Collins, R. A. (1968). "Observation of a Rapidly Pulsating Radio Source". Nature 217 (5130): 709. Bibcode:1968Natur.217..709H（页面存档备份，存于互联网档案馆）. doi:10.1038/217709a0（页面存档备份，存于互联网档案馆）.
Pacini (1968) Pacini, F. (1968). "Rotating Neutron Stars, Pulsars and Supernova Remnants". Nature 219 (5150): 145. Bibcode:1968Natur.219..145P（页面存档备份，存于互联网档案馆）. doi:10.1038/219145a0.
Gold (1968) Gold, T. (1968). "Rotating Neutron Stars as the Origin of the Pulsating Radio Sources". Nature 218 (5143): 731. Bibcode:1968Natur.218..731G（页面存档备份，存于互联网档案馆）. doi:10.1038/218731a0（页面存档备份，存于互联网档案馆）.
Massive double star is latest test for Einstein’s gravity theory. Ron Cowen. Nature. 25 April 2013 [12 May 2013]. （原始内容存档于2013-06-01）.
A heavyweight for Einstein. Max Planck Institute for Radio Astronomy, Bonn. 25 April 2013 [13 May 2013]. （原始内容存档于2013-06-24）.