Rujukan Messier 67

  1. 1 2 Paunzen, E.; Mermilliod, J.-C. "WEBDA page for open cluster NGC 2682". WEBDA. Dicapai pada 2022-10-12.
  2. 1 2 3 Sarajedini, Ata; Dotter, Aaron; Kirkpatrick, Allison (2009). "Deep 2MASS Photometry of M67 and Calibration of the Main-Sequence J - KS Color Difference as an Age Indicator". The Astrophysical Journal. 698 (2): 1872–1878. arXiv:0904.2907. Bibcode:2009ApJ...698.1872S. doi:10.1088/0004-637X/698/2/1872.
  3. 1 2 3 Yakut, K.; Zima, W.; Kalomeni, B.; Van Winckel, H.; Waelkens, C.; De Cat, P.; Bauwens, E.; Vučković, M.; Saesen, S. (2009). "Close binary and other variable stars in the solar-age Galactic open cluster M 67". Astronomy and Astrophysics. 503 (1): 165. arXiv:0906.4908. Bibcode:2009A&A...503..165Y. doi:10.1051/0004-6361/200911918.
  4. 1 2 3 Majaess, Daniel J.; Turner, David G.; Lane, David J.; Krajci, Tom (2011). "Deep Infrared ZAMS Fits to Benchmark Open Clusters Hosting delta Scuti Stars". Journal of the American Association of Variable Star Observers (Jaavso). 39 (2): 219. arXiv:1102.1705. Bibcode:2011JAVSO..39..219M.
  5. ↑ Martina McGovern. "M67 Open cluster". British Astronomical Association. Dicapai pada 2022-10-12.
  6. ↑ Xiao-Bin Zhang; Rong-Xian Zhang; Zhi-Ping Li (2005). "S1280 and S1284: Two Oscillating Blue Stragglers in the Open Cluster M67". Chinese Journal of Astronomy and Astrophysics. 5 (6): 579–586. Bibcode:2005ChJAA...5..579Z. doi:10.1088/1009-9271/5/6/003.
  7. ↑ Harvey B. Richer; Gregory G. Fahlman; Joanne Rosvick; Rodrigo Ibata (1998). "The White Dwarf Cooling Age of M67". The Astrophysical Journal. 504 (2): L91. arXiv:astro-ph/9806172. Bibcode:1998ApJ...504L..91R. doi:10.1086/311586.
  8. ↑ Jarrod R. Hurley; Onno R. Pols; Sverre J. Aarseth; Christopher A. Tout (2005). "A Complete N-body Model of the Old Open Cluster M67". Monthly Notices of the Royal Astronomical Society. 363 (1): 293–314. arXiv:astro-ph/0507239. Bibcode:2005MNRAS.363..293H. doi:10.1111/j.1365-2966.2005.09448.x.
  9. ↑ W. L. Sanders (1977). "Membership of the open cluster M67". Astronomy & Astrophysics Supplement Series. 27: 89–116. Bibcode:1977A&AS...27...89S.
  10. ↑ "Did Our Solar System Originate in a Distant Star Cluster?" (dalam bahasa Inggeris). Daily Galaxy. 30 September 2014. Diarkibkan daripada yang asal pada 10 May 2016. Dicapai pada 30 March 2016.
  11. ↑ Pichardo, Bárbara; Moreno, Edmundo; Allen, Christine; Bedin, Luigi R.; Bellini, Andrea; Pasquini, Luca (February 2012). "The Sun was not born in M 67". The Astronomical Journal. 143 (3): 73. arXiv:1201.0987. Bibcode:2012AJ....143...73P. doi:10.1088/0004-6256/143/3/73. article ID 73.
  12. ↑ Ch. Bonatto; E. Bica (2003). "Mass segregation in M67 with 2MASS" (PDF). Astronomy and Astrophysics. 405 (2): 525. Bibcode:2003A&A...405..525B. doi:10.1051/0004-6361:20030205.
  13. ↑ Sydney A. Barnes; Jörg Weingrill; Dario Fritzewski; Klaus G. Strassmeier; Imants Platais (2016). "Rotation periods for cool stars in the 4 Gyr-old open cluster M67, the solar-stellar connection, and the applicability of gyrochronology to at least solar age". The Astrophysical Journal. 823 (1): 16. arXiv:1603.09179. Bibcode:2016ApJ...823...16B. doi:10.3847/0004-637X/823/1/16.
  14. 1 2 "Stars nearly as old as Sun found to have similar spin rates" (dalam bahasa Inggeris). Astronomy Now. 17 May 2016.