特超巨星 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "特超巨星" in Chinese language version.

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arxiv.org

"假如质量损失是通过间歇的爆发性恒星风实现的，它肯定是由连续的辐射压驱动的超级爱丁顿风暴（e.g., electron scattering opacity），并且不会持续进行。（Owocki, Gayley & Shaviv 2004, hereafter OGS; Belyanin 1999; Quinn & Paczynski 1985）"Owocki, S. P.; Allard Jan van Marle. Luminous Blue Variables & Mass Loss near the Eddington Limit. Bresolin, Fabio; Crowther, Paul Joachim Puls; Puls, Joachim (编). Proceedings IAU Symposium No. 250, 2008. International Astronomical Union. 2008 [2010-02-05]. doi:10.1017/S1743921308020358.
On the nature of the galactic early-B hypergiants (PDF). Astronomy & Astrophysics. [2012-05-18]. （原始内容存档 (PDF)于2021-08-01）.
Yellow and Red Supergiants in the Magellanic Clouds. Astrophysical Journal. [2012-05-21]. （原始内容存档于2021-03-11）.

de Jager, Cornelis. The yellow hypergiants. Astronomy and Astrophysics Review. 1998-03-01, 8 (3). Bibcode:1998A&ARv...8..145D. ISSN 0935-4956. doi:10.1007/s001590050009.
"假如质量损失是通过间歇的爆发性恒星风实现的，它肯定是由连续的辐射压驱动的超级爱丁顿风暴（e.g., electron scattering opacity），并且不会持续进行。（Owocki, Gayley & Shaviv 2004, hereafter OGS; Belyanin 1999; Quinn & Paczynski 1985）"Owocki, S. P.; Allard Jan van Marle. Luminous Blue Variables & Mass Loss near the Eddington Limit. Bresolin, Fabio; Crowther, Paul Joachim Puls; Puls, Joachim (编). Proceedings IAU Symposium No. 250, 2008. International Astronomical Union. 2008 [2010-02-05]. doi:10.1017/S1743921308020358.
S. P. Owocki; K. G. Gayley; N. J. Shaviv. A porosity-length formalism for photon-tiring limited mass loss from stars above the Eddington limit. Astrophysical Journal. 2004, 616: 525–541 [2009-09-04]. doi:10.1086/424910. （原始内容存档于2015-11-06）.
N. Smith; S. P. Owocki. On the role of continuum driven eruptions in the evolution of very massive stars and population III stars. Astrophysical Journal. 2006, 645: L45–L48 [2009-09-04]. doi:10.1086/506523. （原始内容存档于2019-09-03）.

Light variations of α Cygni variables in the Magellanic Clouds (PDF). The Journal of Astrophysical Data. [2012-05-21]. （原始内容存档 (PDF)于2014-12-20）.

S. P. Owocki; K. G. Gayley; N. J. Shaviv. A porosity-length formalism for photon-tiring limited mass loss from stars above the Eddington limit. Astrophysical Journal. 2004, 616: 525–541 [2009-09-04]. doi:10.1086/424910. （原始内容存档于2015-11-06）.
N. Smith; S. P. Owocki. On the role of continuum driven eruptions in the evolution of very massive stars and population III stars. Astrophysical Journal. 2006, 645: L45–L48 [2009-09-04]. doi:10.1086/506523. （原始内容存档于2019-09-03）.
On the nature of the galactic early-B hypergiants (PDF). Astronomy & Astrophysics. [2012-05-18]. （原始内容存档 (PDF)于2021-08-01）.
Light variations of α Cygni variables in the Magellanic Clouds (PDF). The Journal of Astrophysical Data. [2012-05-21]. （原始内容存档 (PDF)于2014-12-20）.
Yellow and Red Supergiants in the Magellanic Clouds. Astrophysical Journal. [2012-05-21]. （原始内容存档于2021-03-11）.