M67 (疏散星團) (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "M67 (疏散星團)" in Chinese language version.

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10harvard.edu

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57^th place

6web.archive.org

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6doi.org

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4arxiv.org

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1univie.ac.at

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1britastro.org

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1dailygalaxy.com

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1aanda.org

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1astronomynow.com

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aanda.org

Ch. Bonatto & E. Bica. Mass segregation in M67 with 2MASS (PDF). Astronomy and Astrophysics. 2003, 405 (2): 525 [2008-03-25]. Bibcode:2003A&A...405..525B. doi:10.1051/0004-6361:20030205 . （原始内容 (PDF)存档于2019-06-15）.

arxiv.org

Harvey B. Richer; Gregory G. Fahlman; Joanne Rosvick; Rodrigo Ibata. The White Dwarf Cooling Age of M67. The Astrophysical Journal. 1998, 504 (2): L91. Bibcode:1998ApJ...504L..91R. arXiv:astro-ph/9806172 . doi:10.1086/311586.
Jarrod R. Hurley; Onno R. Pols; Sverre J. Aarseth; Christopher A. Tout. A Complete N-body Model of the Old Open Cluster M67. Monthly Notices of the Royal Astronomical Society. 2005, 363 (1): 293–314. Bibcode:2005MNRAS.363..293H. arXiv:astro-ph/0507239 . doi:10.1111/j.1365-2966.2005.09448.x.
Pichardo, Bárbara; Moreno, Edmundo; Allen, Christine; Bedin, Luigi R.; Bellini, Andrea; Pasquini, Luca. The Sun was not born in M 67. The Astronomical Journal. February 2012, 143 (3): 73. Bibcode:2012AJ....143...73P. arXiv:1201.0987 . doi:10.1088/0004-6256/143/3/73. article ID 73.
Sydney A. Barnes; Jörg Weingrill; Dario Fritzewski; Klaus G. Strassmeier; Imants Platais. 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. 2016, 823 (1): 16. Bibcode:2016ApJ...823...16B. arXiv:1603.09179 . doi:10.3847/0004-637X/823/1/16.

astronomynow.com

Stars nearly as old as Sun found to have similar spin rates. Astronomy Now. 17 May 2016 [2022-04-09]. （原始内容存档于2021-05-18）（英语）.

britastro.org

Martina McGovern [1] （页面存档备份，存于互联网档案馆）

dailygalaxy.com

Did Our Solar System Originate in a Distant Star Cluster?. Daily Galaxy. 30 September 2014 [30 March 2016]. （原始内容存档于10 May 2016）（英语）.

doi.org

Xiao-Bin Zhang; Rong-Xian Zhang & Zhi-Ping Li. S1280 and S1284: Two Oscillating Blue Stragglers in the Open Cluster M67. Chinese Journal of Astronomy and Astrophysics. 2005, 5 (6): 579–586. Bibcode:2005ChJAA...5..579Z. doi:10.1088/1009-9271/5/6/003.
Harvey B. Richer; Gregory G. Fahlman; Joanne Rosvick; Rodrigo Ibata. The White Dwarf Cooling Age of M67. The Astrophysical Journal. 1998, 504 (2): L91. Bibcode:1998ApJ...504L..91R. arXiv:astro-ph/9806172 . doi:10.1086/311586.
Jarrod R. Hurley; Onno R. Pols; Sverre J. Aarseth; Christopher A. Tout. A Complete N-body Model of the Old Open Cluster M67. Monthly Notices of the Royal Astronomical Society. 2005, 363 (1): 293–314. Bibcode:2005MNRAS.363..293H. arXiv:astro-ph/0507239 . doi:10.1111/j.1365-2966.2005.09448.x.
Pichardo, Bárbara; Moreno, Edmundo; Allen, Christine; Bedin, Luigi R.; Bellini, Andrea; Pasquini, Luca. The Sun was not born in M 67. The Astronomical Journal. February 2012, 143 (3): 73. Bibcode:2012AJ....143...73P. arXiv:1201.0987 . doi:10.1088/0004-6256/143/3/73. article ID 73.
Ch. Bonatto & E. Bica. Mass segregation in M67 with 2MASS (PDF). Astronomy and Astrophysics. 2003, 405 (2): 525 [2008-03-25]. Bibcode:2003A&A...405..525B. doi:10.1051/0004-6361:20030205 . （原始内容 (PDF)存档于2019-06-15）.
Sydney A. Barnes; Jörg Weingrill; Dario Fritzewski; Klaus G. Strassmeier; Imants Platais. 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. 2016, 823 (1): 16. Bibcode:2016ApJ...823...16B. arXiv:1603.09179 . doi:10.3847/0004-637X/823/1/16.

harvard.edu

ui.adsabs.harvard.edu

Xiao-Bin Zhang; Rong-Xian Zhang & Zhi-Ping Li. S1280 and S1284: Two Oscillating Blue Stragglers in the Open Cluster M67. Chinese Journal of Astronomy and Astrophysics. 2005, 5 (6): 579–586. Bibcode:2005ChJAA...5..579Z. doi:10.1088/1009-9271/5/6/003.
Harvey B. Richer; Gregory G. Fahlman; Joanne Rosvick; Rodrigo Ibata. The White Dwarf Cooling Age of M67. The Astrophysical Journal. 1998, 504 (2): L91. Bibcode:1998ApJ...504L..91R. arXiv:astro-ph/9806172 . doi:10.1086/311586.
Jarrod R. Hurley; Onno R. Pols; Sverre J. Aarseth; Christopher A. Tout. A Complete N-body Model of the Old Open Cluster M67. Monthly Notices of the Royal Astronomical Society. 2005, 363 (1): 293–314. Bibcode:2005MNRAS.363..293H. arXiv:astro-ph/0507239 . doi:10.1111/j.1365-2966.2005.09448.x.
W. L. Sanders. Membership of the open cluster M67. Astronomy & Astrophysics Supplement Series. 1977, 27: 89–116. Bibcode:1977A&AS...27...89S.
Pichardo, Bárbara; Moreno, Edmundo; Allen, Christine; Bedin, Luigi R.; Bellini, Andrea; Pasquini, Luca. The Sun was not born in M 67. The Astronomical Journal. February 2012, 143 (3): 73. Bibcode:2012AJ....143...73P. arXiv:1201.0987 . doi:10.1088/0004-6256/143/3/73. article ID 73.
Ch. Bonatto & E. Bica. Mass segregation in M67 with 2MASS (PDF). Astronomy and Astrophysics. 2003, 405 (2): 525 [2008-03-25]. Bibcode:2003A&A...405..525B. doi:10.1051/0004-6361:20030205 . （原始内容 (PDF)存档于2019-06-15）.
Sydney A. Barnes; Jörg Weingrill; Dario Fritzewski; Klaus G. Strassmeier; Imants Platais. 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. 2016, 823 (1): 16. Bibcode:2016ApJ...823...16B. arXiv:1603.09179 . doi:10.3847/0004-637X/823/1/16.

adsabs.harvard.edu

Sarajedini, Ata; Dotter, Aaron; Kirkpatrick, Allison "Deep 2MASS Photometry of M67 and Calibration of the Main-Sequence J – KS Color Difference as an Age Indicator", AJ, 2009
Yakut, K.; Zima, W.; Kalomeni, B.; van Winckel, H.; Waelkens, C.; De Cat, P.; Bauwens, E.; Vučković, M.; Saesen, S.; Le Guillou, L.; Parmaksızoğlu, M.; Uluç, K.; Khamitov, I.; Raskin, G.; Aerts, C."Close binary and other variable stars in the solar-age Galactic open cluster M 67", A&A, 2009
Majaess, D.; Turner, D.; Lane, D.; Krajci, T. "Deep Infrared ZAMS Fits to Benchmark Open Clusters Hosting delta Scuti Stars" （页面存档备份，存于互联网档案馆）, Journal of the American Association of Variable Star Observers, 2011

univie.ac.at

Paunzen, E., Mermilliod, J.-C. "WEBDA: M67" （页面存档备份，存于互联网档案馆）

web.archive.org

Paunzen, E., Mermilliod, J.-C. "WEBDA: M67" （页面存档备份，存于互联网档案馆）
Majaess, D.; Turner, D.; Lane, D.; Krajci, T. "Deep Infrared ZAMS Fits to Benchmark Open Clusters Hosting delta Scuti Stars" （页面存档备份，存于互联网档案馆）, Journal of the American Association of Variable Star Observers, 2011
Martina McGovern [1] （页面存档备份，存于互联网档案馆）
Did Our Solar System Originate in a Distant Star Cluster?. Daily Galaxy. 30 September 2014 [30 March 2016]. （原始内容存档于10 May 2016）（英语）.
Ch. Bonatto & E. Bica. Mass segregation in M67 with 2MASS (PDF). Astronomy and Astrophysics. 2003, 405 (2): 525 [2008-03-25]. Bibcode:2003A&A...405..525B. doi:10.1051/0004-6361:20030205 . （原始内容 (PDF)存档于2019-06-15）.
Stars nearly as old as Sun found to have similar spin rates. Astronomy Now. 17 May 2016 [2022-04-09]. （原始内容存档于2021-05-18）（英语）.