Wilkins, Stephen M.; Trentham, Neil; Hopkins, Andrew M. (2008-02-29). “The evolution of stellar mass and the implied star formation history” (英語). Monthly Notices of the Royal Astronomical Society385: 687-694. doi:10.1111/j.1365-2966.2008.12885.x. Wilkins, Stephen M.; Trentham, Neil; Hopkins, Andrew M. (10 January 2008). "The Evolution of Stellar Mass and the Implied Star Formation History" (英語). arXiv:0801.1594。 z = 3 では恒星の質量密度は現在のおよそ 1/10 となる (Fig. 1)。
doi.org
Wilkins, Stephen M.; Trentham, Neil; Hopkins, Andrew M. (2008-02-29). “The evolution of stellar mass and the implied star formation history” (英語). Monthly Notices of the Royal Astronomical Society385: 687-694. doi:10.1111/j.1365-2966.2008.12885.x. Wilkins, Stephen M.; Trentham, Neil; Hopkins, Andrew M. (10 January 2008). "The Evolution of Stellar Mass and the Implied Star Formation History" (英語). arXiv:0801.1594。 z = 3 では恒星の質量密度は現在のおよそ 1/10 となる (Fig. 1)。
Halley, Edmund (1721). “Of the Infinity of the Sphere of Fix'd Stars” (英語). Philosophical Transactions31: 22-24. doi:10.1098/rstl.1720.0006. Halley, Edmund (1721). “Of the Number, Order, and Light of the Fix'd Stars” (英語). Philosophical Transactions31: 24-26. doi:10.1098/rstl.1720.0007.
Lord Kelvin (August 1901). “XII. On ether and gravitational matter through infinite space” (英語). Philosophical Magazine, Series 62: 161-177. doi:10.1080/14786440109462676.
Wesson, Paul S. (February 1991). “Olbers's paradox and the spectral intensity of the extragalactic background light” (英語). Astrophysical Journal, Part 1367: 399-406. doi:10.1086/169638.
