金屬量 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "金屬量" in Chinese language version.

refsWebsite

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arxiv.org

R. A. E. Fosbury; et al. Massive Star Formation in a Gravitationally Lensed H II Galaxy at z = 3.357. Astrophysical Journal. 2003, 596 (1): 797–809 [2007-08-19]. （原始内容存档于2016-06-02）.
A. Heger, S. E. Woosley. The Nucleosynthetic Signature of Population III. Astrophysical Journal. 2002, 567 (1): 532–543 [2007-08-19]. （原始内容存档于2016-01-10）.

Lauren J. Bryant. What Makes Stars Tick. Indiana University Research & Creative Activity. [2005-09-07]. （原始内容存档于2016-05-16）.

John C. Martin. What we learn from a star's metal content. New Analysis RR Lyrae Kinematics in the Solar Neighborhood. [2005-09-07]. （原始内容存档于2009-01-06）.
John C. Martin: What we learn from a star's metal content. 互联网档案馆的存檔，存档日期2009-01-06.

John C. Martin. What we learn from a star's metal content. New Analysis RR Lyrae Kinematics in the Solar Neighborhood. [2005-09-07]. （原始内容存档于2009-01-06）.
Lauren J. Bryant. What Makes Stars Tick. Indiana University Research & Creative Activity. [2005-09-07]. （原始内容存档于2016-05-16）.
John C. Martin: What we learn from a star's metal content. 互联网档案馆的存檔，存档日期2009-01-06.
Charles H. Lineweaver. An Estimate of the Age Distribution of Terrestrial Planets in the Universe: Quantifying Metallicity as a Selection Effect. University of New South Wales. 2000 [2006-07-23]. （原始内容存档于2020-05-12）.
R. A. E. Fosbury; et al. Massive Star Formation in a Gravitationally Lensed H II Galaxy at z = 3.357. Astrophysical Journal. 2003, 596 (1): 797–809 [2007-08-19]. （原始内容存档于2016-06-02）.
A. Heger, S. E. Woosley. The Nucleosynthetic Signature of Population III. Astrophysical Journal. 2002, 567 (1): 532–543 [2007-08-19]. （原始内容存档于2016-01-10）.
Formation of the First Stars and Galaxies. [2009-08-20]. （原始内容存档于2021-05-15）.