오리온 성운 (Korean Wikipedia)

Analysis of information sources in references of the Wikipedia article "오리온 성운" in Korean language version.

refsWebsite

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5,388^th place

2,373^rd place

1cfa-harvard.edu

low place

low place

1web.archive.org

1^st place

1^st place

1clarkvision.com

low place

low place

arxiv.org

Reid, M. J.; 외. (2009). “Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions”. 《Astrophysical Journal》 700 (1): 137–148. arXiv:0902.3913. Bibcode:2009ApJ...700..137R. doi:10.1088/0004-637X/700/1/137.
Hirota, Tomoya; 외. (2007년). “Distance to Orion KL Measured with VERA”. 《Publications of the Astronomical Society of Japan》 59 (5): 897–903. arXiv:0705.3792. Bibcode:2007PASJ...59..897H. doi:10.1093/pasj/59.5.897.

cfa-harvard.edu

Press release, "Astronomers Spot The Great Orion Nebula's Successor 보관됨 2006-02-18 - 웨이백 머신", Harvard-Smithsonian Center for Astrophysics, 2006.

clarkvision.com

Clark, Roger (2004년 3월 28일). “Surface Brightness of Deep Sky Objects”. 2013년 6월 29일에 확인함. . The conversion to nits is based on 0 magnitude being 2.08 microlux.

doi.org

dx.doi.org

Reid, M. J.; 외. (2009). “Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions”. 《Astrophysical Journal》 700 (1): 137–148. arXiv:0902.3913. Bibcode:2009ApJ...700..137R. doi:10.1088/0004-637X/700/1/137.
Hirota, Tomoya; 외. (2007년). “Distance to Orion KL Measured with VERA”. 《Publications of the Astronomical Society of Japan》 59 (5): 897–903. arXiv:0705.3792. Bibcode:2007PASJ...59..897H. doi:10.1093/pasj/59.5.897.

harvard.edu

adsabs.harvard.edu

Reid, M. J.; 외. (2009). “Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions”. 《Astrophysical Journal》 700 (1): 137–148. arXiv:0902.3913. Bibcode:2009ApJ...700..137R. doi:10.1088/0004-637X/700/1/137.
Hirota, Tomoya; 외. (2007년). “Distance to Orion KL Measured with VERA”. 《Publications of the Astronomical Society of Japan》 59 (5): 897–903. arXiv:0705.3792. Bibcode:2007PASJ...59..897H. doi:10.1093/pasj/59.5.897.

seds.org

spider.seds.org

“NGC 1976 = M42”. 《SEDS.org》. 2009년 12월 13일에 확인함.

web.archive.org

Press release, "Astronomers Spot The Great Orion Nebula's Successor 보관됨 2006-02-18 - 웨이백 머신", Harvard-Smithsonian Center for Astrophysics, 2006.