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For an in-depth discussion of Pleiades parallax measurements, see section 6.3 of van Leeuwen, F. (2009). “Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue”. Astronomy and Astrophysics497 (1): 209-242. arXiv:0902.1039. Bibcode: 2009A&A...497..209V. doi:10.1051/0004-6361/200811382.
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For an in-depth discussion of Pleiades parallax measurements, see section 6.3 of van Leeuwen, F. (2009). “Parallaxes and proper motions for 20 open clusters as based on the new Hipparcos catalogue”. Astronomy and Astrophysics497 (1): 209-242. arXiv:0902.1039. Bibcode: 2009A&A...497..209V. doi:10.1051/0004-6361/200811382.
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Porter, J. M.; Rivinius, T. (2003). “Classical Be Stars”. Publications of the Astronomical Society of the Pacific115 (812): 1153-1170. Bibcode: 2003PASP..115.1153P. doi:10.1086/378307.
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Kaler, J. B.. “PLEIONE (28 Tauri)”. University of Illinois. 2010年6月11日閲覧。 Kaler acknowledges a distance of 385ly to Pleione, an estimate that is likely derived from the Hipparcos Catalogue published in 1997. Any significant change in astrometric calculations could impact other calculations referenced in this article.