Ross 248 (Hungarian Wikipedia)

Analysis of information sources in references of the Wikipedia article "Ross 248" in Hungarian language version.

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  • Schroeder, Daniel J. (2000). „A Search for Faint Companions to Nearby Stars Using the Wide Field Planetary Camera 2”. The Astronomical Journal 119, 906–922. o. DOI:10.1086/301227. 
  • Cenarro, A. J.. „Medium-resolution Isaac Newton Telescope Library of Empirical Spectra – II. The Stellar Atmospheric Parameters”. Monthly Notices of the Royal Astronomical Society 374 (2), 664–690. o. DOI:10.1111/j.1365-2966.2006.11196.x. 
  • Leggett, S. K. (1992. September). „Infrared colors of low-mass stars”. Astrophysical Journal Supplement Series 82 (1), 351–394. o. DOI:10.1086/191720. 
  • Lépine, Sébastien; Shara, Michael M (2005. March). „A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog)”. The Astronomical Journal 129 (3), 1483–1522. o. DOI:10.1086/427854. 
  • Johnson, H. M.; Wright, C. D. (1983. November). „Predicted infrared brightness of stars within 25 parsecs of the sun”. Astrophysical Journal Supplement Series 53, 643–711. o. DOI:10.1086/190905.  Lásd 705. o.
  • Reiners, A.; Basri, G. (2007. February). „The First Direct Measurements of Surface Magnetic Fields on Very Low Mass Stars”. The Astrophysical Journal 656 (2), 1121–1135. o. DOI:10.1086/510304. 
  • Ross, Frank E. (1926. February). „New proper-motion stars, (second list)”. Astronomical Journal 36 (856), 124-128. o. DOI:10.1086/104699. 
  • Weis, Edward W. (1994. March). „Long term variability in dwarf M stars”. Astronomical Journal 107 (3), 1135-1140. o. DOI:10.1086/116925. 
  • Lippincott, S. L. (1978. July). „Astrometric search for unseen stellar and sub-stellar companions to nearby stars and the possibility of their detection”. Space Science Reviews 22, 153-189. o. DOI:10.1007/BF00212072. 
  • Hinz, Joannah L. et al (2002. February). „A Near-Infrared, Wide-Field, Proper-Motion Search for Brown Dwarfs”. The Astronomical Journal 123 (4), 2027–2032. o. DOI:10.1086/339555. 

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