^ 2.02.12.2John Stansberry, Will Grundy, Mike Brown, Dale Cruikshank, John Spencer, David Trilling, Jean-Luc Margot. Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope. University of Arizona, Lowell Observatory, California Institute of Technology, NASA Ames Research Center, Southwest Research Institute, Cornell University. 2007 [2008-10-18]. (原始内容于2016-10-09).
^Wm. Robert Johnston. List of Known Trans-Neptunian Objects. Johnston's Archive. 22 August 2008 [2006-12-17]. (原始内容于2008-09-28).
^Fernández, Yanga R.; Jewitt, David C.; Sheppard, Scott S. Thermal Properties of Centaurs Asbolus and Chiron. The Astronomical Journal. 2002, 112 (2): 1050–1055 [2004-10-06]. doi:10.1086/338436.引文使用过时参数coauthors (帮助)
^Centaur's Bright Surface Spot Could be Crater of Fresh Ice. Hubblesite (STScI-2000-31). September 14, 2000 [2004-04-12]. (原始内容存档于2012-07-16).
^ 6.06.16.2Horner, J.; Evans, N.W.; Bailey, M. E. Simulations of the Population of Centaurs I: The Bulk Statistics. 2004 [2008-09-01]. (原始内容于2019-08-10).引文使用过时参数coauthors (帮助)
^The perihelion (q) of twenty-two clones of Centaur Asbolus. [2009-04-26]. (Solex 10) (页面存档备份,存于互联网档案馆)
^Three clones of Centaur 8405 Asbolus making passes within 450Gm. [2009-05-02].[失效連結] (Solex 10) Archived 2009-04-29 at WebCite
外部連結
Orbital simulation from JPL (Java) / Ephemeris (页面存档备份,存于互联网档案馆)