星系群 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "星系群" in Chinese language version.

refsWebsite

Global rank Chinese rank

1^st place

18^th place

57^th place

69^th place

254^th place

2^nd place

23^rd place

3,034^th place

2,034^th place

8,860^th place

6,987^th place

4,653^rd place

4,945^th place

670^th place

845^th place

arxiv.org

Brownstein, J. R.; Moffat, J. W. Galaxy Cluster Masses Without Non-Baryonic Dark Matter. Monthly Notices of the Royal Astronomical Society. 2006, 367: 527–540. Bibcode:2006MNRAS.367..527B. arXiv:astro-ph/0507222 . doi:10.1111/j.1365-2966.2006.09996.x.
Markevitch; Gonzalez; Clowe; Vikhlinin; David; Forman; Jones; Murray; Tucker. Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56. Astrophys.J. 2003, 606 (2): 819–824. Bibcode:2004ApJ...606..819M. arXiv:astro-ph/0309303 . doi:10.1086/383178.
Coe, Dan; Benítez, Narciso; Broadhurst, Tom; Moustakas, Leonidas A. A High-resolution Mass Map of Galaxy Cluster Substructure: LensPerfect Analysis of A1689. The Astrophysical Journal. 2010, 723: 1678. Bibcode:2010ApJ...723.1678C. arXiv:1005.0398 . doi:10.1088/0004-637X/723/2/1678.
McDermott, Samuel D.; Yu, Hai-Bo; Zurek, Kathryn M. Turning off the lights: How dark is dark matter?. Physical Review D. 2011, 83: 063509. Bibcode:2011PhRvD..83f3509M. arXiv:1011.2907 . doi:10.1103/PhysRevD.83.063509.
Brownstein, J. R.; Moffat, J. W. The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter. Monthly Notices of the Royal Astronomical Society. 2007, 382: 29–47. Bibcode:2007MNRAS.382...29B. arXiv:astro-ph/0702146v3 . doi:10.1111/j.1365-2966.2007.12275.x.

Brownstein, J. R.; Moffat, J. W. Galaxy Cluster Masses Without Non-Baryonic Dark Matter. Monthly Notices of the Royal Astronomical Society. 2006, 367: 527–540. Bibcode:2006MNRAS.367..527B. arXiv:astro-ph/0507222 . doi:10.1111/j.1365-2966.2006.09996.x.
Markevitch; Gonzalez; Clowe; Vikhlinin; David; Forman; Jones; Murray; Tucker. Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56. Astrophys.J. 2003, 606 (2): 819–824. Bibcode:2004ApJ...606..819M. arXiv:astro-ph/0309303 . doi:10.1086/383178.
Coe, Dan; Benítez, Narciso; Broadhurst, Tom; Moustakas, Leonidas A. A High-resolution Mass Map of Galaxy Cluster Substructure: LensPerfect Analysis of A1689. The Astrophysical Journal. 2010, 723: 1678. Bibcode:2010ApJ...723.1678C. arXiv:1005.0398 . doi:10.1088/0004-637X/723/2/1678.
McDermott, Samuel D.; Yu, Hai-Bo; Zurek, Kathryn M. Turning off the lights: How dark is dark matter?. Physical Review D. 2011, 83: 063509. Bibcode:2011PhRvD..83f3509M. arXiv:1011.2907 . doi:10.1103/PhysRevD.83.063509.
Brownstein, J. R.; Moffat, J. W. The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter. Monthly Notices of the Royal Astronomical Society. 2007, 382: 29–47. Bibcode:2007MNRAS.382...29B. arXiv:astro-ph/0702146v3 . doi:10.1111/j.1365-2966.2007.12275.x.

Huge Map of the Distant Universe Reaches Halfway Point. ESO. [2 April 2013]. （原始内容存档于2021-01-26）.
The Most Distant Mature Galaxy Cluster. ESO Science Release. ESO. [9 March 2011]. （原始内容存档于2021-03-09）.

Brownstein, J. R.; Moffat, J. W. Galaxy Cluster Masses Without Non-Baryonic Dark Matter. Monthly Notices of the Royal Astronomical Society. 2006, 367: 527–540. Bibcode:2006MNRAS.367..527B. arXiv:astro-ph/0507222 . doi:10.1111/j.1365-2966.2006.09996.x.
Markevitch; Gonzalez; Clowe; Vikhlinin; David; Forman; Jones; Murray; Tucker. Direct constraints on the dark matter self-interaction cross-section from the merging galaxy cluster 1E0657-56. Astrophys.J. 2003, 606 (2): 819–824. Bibcode:2004ApJ...606..819M. arXiv:astro-ph/0309303 . doi:10.1086/383178.
Coe, Dan; Benítez, Narciso; Broadhurst, Tom; Moustakas, Leonidas A. A High-resolution Mass Map of Galaxy Cluster Substructure: LensPerfect Analysis of A1689. The Astrophysical Journal. 2010, 723: 1678. Bibcode:2010ApJ...723.1678C. arXiv:1005.0398 . doi:10.1088/0004-637X/723/2/1678.
McDermott, Samuel D.; Yu, Hai-Bo; Zurek, Kathryn M. Turning off the lights: How dark is dark matter?. Physical Review D. 2011, 83: 063509. Bibcode:2011PhRvD..83f3509M. arXiv:1011.2907 . doi:10.1103/PhysRevD.83.063509.
Brownstein, J. R.; Moffat, J. W. The Bullet Cluster 1E0657-558 evidence shows Modified Gravity in the absence of Dark Matter. Monthly Notices of the Royal Astronomical Society. 2007, 382: 29–47. Bibcode:2007MNRAS.382...29B. arXiv:astro-ph/0702146v3 . doi:10.1111/j.1365-2966.2007.12275.x.

A scattering of spiral and elliptical galaxies. ESA/Hubble Picture of the Week. [25 September 2013]. （原始内容存档于2020-09-19）.

UTK Physics Dept. Groups of Galaxies. University of Tennessee, Knoville. [September 27, 2012]. （原始内容存档于2012-06-24）.

A scattering of spiral and elliptical galaxies. ESA/Hubble Picture of the Week. [25 September 2013]. （原始内容存档于2020-09-19）.
Huge Map of the Distant Universe Reaches Halfway Point. ESO. [2 April 2013]. （原始内容存档于2021-01-26）.
UTK Physics Dept. Groups of Galaxies. University of Tennessee, Knoville. [September 27, 2012]. （原始内容存档于2012-06-24）.
Mike Irwin. The Local Group. [2009-11-07]. （原始内容存档于2019-06-19）.
The Most Distant Mature Galaxy Cluster. ESO Science Release. ESO. [9 March 2011]. （原始内容存档于2021-03-09）.