อ้างอิง ของ ดาวกัปไตน์

  1. 1 2 3 4 5 6 7 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
  2. 1 2 3 Koen, C.; และคณะ (April 2010), "UBV(RI)C JHK observations of Hipparcos-selected nearby stars", Monthly Notices of the Royal Astronomical Society, 403 (4): 1949–1968, Bibcode:2010MNRAS.403.1949K, doi:10.1111/j.1365-2966.2009.16182.x
  3. 1 2 3 4 "V* VZ Pic -- Variable Star", SIMBAD, Centre de Données astronomiques de Strasbourg, สืบค้นเมื่อ 2009-10-14.
  4. 1 2 "VZ Pic", General Catalogue of Variable Stars, Sternberg Astronomical Institute, Moscow, Russia, สืบค้นเมื่อ 2009-10-14
  5. ↑ Nordström, B.; และคณะ (May 2004), "The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs", Astronomy and Astrophysics, 418 (3): 989–1019, arXiv:astro-ph/0405198, Bibcode:2004A&A...418..989N, doi:10.1051/0004-6361:20035959
  6. 1 2 3 4 5 6 7 Kotoneva, E.; และคณะ (2005), "A study of Kapteyn's star", Astronomy & Astrophysics, 438 (3): 957–962, Bibcode:2005A&A...438..957K, doi:10.1051/0004-6361:20042287.
  7. ↑ Demory, B.-O.; และคณะ (October 2009), "Mass-radius relation of low and very low-mass stars revisited with the VLTI", Astronomy and Astrophysics, 505 (1): 205–215, arXiv:0906.0602, Bibcode:2009A&A...505..205D, doi:10.1051/0004-6361/200911976
  8. ↑ Houdebine, E. R. (September 2010), "Observation and modelling of main-sequence star chromospheres - XIV. Rotation of dM1 stars", Monthly Notices of the Royal Astronomical Society, 407 (3): 1657–1673, Bibcode:2010MNRAS.407.1657H, doi:10.1111/j.1365-2966.2010.16827.x
  9. ↑ Kapteyn, J. C. (1898), "Stern mit grösster bislang bekannter Eigenbewegung", Astronomische Nachrichten, 145 (9–10): 159–160, Bibcode:1897AN....145..159K, doi:10.1002/asna.18981450906.
  10. 1 2 3 Kaler, James B. (2002), "Kapteyn's Star", The Hundred Greatest Stars, Copernicus Books, pp. 108–109.
  11. ↑ Barnard, E. E. (1916), "A small star with large proper motion", Astronomical Journal, 29 (695): 181, Bibcode:1916AJ.....29..181B, doi:10.1086/104156.
  12. 1 2 3 Anglada-Escudé, Guillem; และคณะ (2014), Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf, arXiv:1406.0818
  13. ↑ Bobylev, Vadim V. (March 2010), "Searching for Stars Closely Encountering with the Solar System", Astronomy Letters, 36 (3): 220–226, arXiv:1003.2160, Bibcode:2010AstL...36..220B, doi:10.1134/S1063773710030060.
  14. ↑ Woolf, Vincent M.; Wallerstein, George (January 2005), "Metallicity measurements using atomic lines in M and K dwarf stars", Monthly Notices of the Royal Astronomical Society, 356 (3): 963–968, arXiv:astro-ph/0410452, Bibcode:2005MNRAS.356..963W, doi:10.1111/j.1365-2966.2004.08515.x
  15. ↑ The abundance is given by taking the metallicity to the power of 10. From Woolf and Wallerstein (2005), [M/H] ≈ –0.86 dex. Thus:10–0.86 = 0.138
  16. ↑ Woolf, V. M.; Wallerstein, G. (2004), "Chemical abundance analysis of Kapteyn's Star", Monthly Notices of the Royal Astronomical Society, 350 (2): 575–579, Bibcode:2004MNRAS.350..575W, doi:10.1111/j.1365-2966.2004.07671.x.
  17. ↑ Eggen, O. J. (December 1996), "The Ross 451 Group of Halo Stars", Astronomical Journal, 112: 2661, Bibcode:1996AJ....112.2661E, doi:10.1086/118210
  18. ↑ Wylie-de Boer, Elizabeth; Freeman, Ken; Williams, Mary (February 2010), "Evidence of Tidal Debris from ω Cen in the Kapteyn Group", The Astronomical Journal, 139 (2): 636–645, arXiv:0910.3735, Bibcode:2010AJ....139..636W, doi:10.1088/0004-6256/139/2/636
  19. ↑ "Backward star ain't from round here", New Scientist, November 4, 2009
  20. ↑ Michtchenko, Tatiana A.; และคณะ (August 2011), "Modeling the secular evolution of migrating planet pairs", Monthly Notices of the Royal Society, 415: 2275, arXiv:1103.5485, Bibcode:2011MNRAS.415.2275MCS1 maint: date and year (link)
  21. ↑ "Sad Kapteyn", Science fiction story released with the announcement of planetary system, Jun 4, 2014, สืบค้นเมื่อ 2014-06-04