WR 22 (Korean Wikipedia)

Analysis of information sources in references of the Wikipedia article "WR 22" in Korean language version.

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  • Van Leeuwen, F. (2007). “Validation of the new Hipparcos reduction”. 《Astronomy and Astrophysics》 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. 
  • Ducati, J. R. (2002). “VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system”. 《CDS/ADC Collection of Electronic Catalogues》 2237. Bibcode:2002yCat.2237....0D. 
  • Cutri, R. M.; Skrutskie, M. F.; Van Dyk, S.; Beichman, C. A.; Carpenter, J. M.; Chester, T.; Cambresy, L.; Evans, T.; Fowler, J.; Gizis, J.; Howard, E.; Huchra, J.; Jarrett, T.; Kopan, E. L.; Kirkpatrick, J. D.; Light, R. M.; Marsh, K. A.; McCallon, H.; Schneider, S.; Stiening, R.; Sykes, M.; Weinberg, M.; Wheaton, W. A.; Wheelock, S.; Zacarias, N. (2003). “VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)”. 《VizieR On-line Data Catalog: II/246. Originally Published in: 2003yCat.2246....0C》 2246. Bibcode:2003yCat.2246....0C. 
  • Gosset, E.; Nazé, Y.; Sana, H.; Rauw, G.; Vreux, J.-M. (2009). “Phase-resolved XMM-Newton observations of the massive WR+O binary WR 22”. 《Astronomy and Astrophysics》 508 (2): 805. Bibcode:2009A&A...508..805G. doi:10.1051/0004-6361/20077981. 
  • Kharchenko, N. V.; Scholz, R.-D.; Piskunov, A. E.; Röser, S.; Schilbach, E. (2007). “Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations”. 《Astronomische Nachrichten》 328 (9): 889. arXiv:0705.0878. Bibcode:2007AN....328..889K. doi:10.1002/asna.200710776. 
  • Gräfener, G.; Hamann, W.-R. (2008). “Mass loss from late-type WN stars and its Z-dependence. Very massive stars approaching the Eddington limit”. 《Astronomy and Astrophysics》 482 (3): 945. arXiv:0803.0866. Bibcode:2008A&A...482..945G. doi:10.1051/0004-6361:20066176. 
  • Parkin, E. R.; Gosset, E. (2011). “Investigating the X-ray emission from the massive WR+O binary WR 22 using 3D hydrodynamical models”. 《Astronomy & Astrophysics》 530: A119. arXiv:1104.2383. Bibcode:2011A&A...530A.119P. doi:10.1051/0004-6361/201016125. 
  • Gagné, M.; Fehon, G.; Savoy, M. R.; Cartagena, C. A.; Cohen, D. H.; Owocki, S. P. (2012). “An X-Ray Survey of Colliding Wind Binaries”. 《Proceedings of a Scientific Meeting in Honor of Anthony F. J. Moffat Held at Auberge du Lac Taureau》 465: 301. arXiv:1205.3510. Bibcode:2012ASPC..465..301G. 
  • Schweickhardt, J.; Schmutz, W.; Stahl, O.; Szeifert, Th.; Wolf, B. (1999). “Revised mass determination of the super massive Wolf-Rayet star WR 22”. 《Astronomy and Astrophysics》 347: 127. Bibcode:1999A&A...347..127S. 

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