Ciemna materia (Polish Wikipedia)

Analysis of information sources in references of the Wikipedia article "Ciemna materia" in Polish language version.

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  • Vera C. Rubin, W. Kent Ford Jr.. Rotation of the Andromeda Nebula from a Spectroscopic Survey of Emission Regions. „The Astrophysical Journal”. 159, s. 379, luty 1970. DOI: 10.1086/150317. Bibcode1970ApJ...159..379R. (ang.). 
  • Douglas Clowe, Marusa Bradac, Anthony H. Gonzalez, Maxim Markevitch, Scott W. Randall, Christine Jones, Dennis Zaritsky. A direct empirical proof of the existence of dark matter. „The Astrophysical Journal Letters + arXiv”. 648 (2), 2006-08-19. DOI: 10.1086/508162. arXiv:astro-ph/0608407. [dostęp 2011-05-07]. (ang.). 
  • E. Komatsu et al.. Five-Year Wilkinson Microwave Anisotropy Probe Observations: Cosmological Interpretation. „The Astrophysical Journal Supplement Series”. 180 (2), s. 330, luty 2009. DOI: 10.1088/0067-0049/180/2/330. (ang.). 
  • S. Perlmutter et al.. Measurements of Ω and Λ from 42 High-Redshift Supernovae. „The Astrophysical Journal”. 517 (2), s. 565, 1999-06-01. DOI: 10.1086/307221. (ang.). 
  • S.W. Allen et al.. Cosmological constraints from the local X-ray luminosity function of the most X-ray-luminous galaxy clusters. „Monthly Notices of the Royal Astronomical Society”. 342 (1), s. 287-298, 2003-06-11. DOI: 10.1046/j.1365-8711.2003.06550.x. (ang.). 
  • Dan Hooper, Lisa Lisa Goodenough. Dark matter annihilation in the Galactic Center as seen by the Fermi Gamma Ray Space Telescope. „Physics Letters B”. 697 (5), s. 412-428, 2011-03-21. DOI: 10.1016/j.physletb.2011.02.029. arXiv:1010.2752. (ang.). 
  • F. Aharonian et al.. A Search for a Dark Matter Annihilation Signal Toward the Canis Major Overdensity with H.E.S.S.. „The Astrophysical Journal”. 691 (1), s. 175–181, 2009-01-20. DOI: 10.1088/0004-637X/691/1/175. (ang.). 
  • AL Peratt and J Green. On the Evolution of Interacting, Magnetized, Galactic Plasmas. „Astrophysics and Space Science”. 91, s. 19–33, 1983. DOI: 10.1007/BF00650210. Bibcode1983Ap&SS..91...19P. 

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