中等質量黑洞 (Chinese Wikipedia)

Analysis of information sources in references of the Wikipedia article "中等質量黑洞" in Chinese language version.

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arxiv.org

Gebhardt, Karl; Rich, R. M.; Ho, Luis C., An Intermediate-Mass Black Hole in the Globular Cluster G1: Improved Significance from New Keck and Hubble Space Telescope Observations, The Astrophysical Journal, December 2005, 634 (2): 1093–1102, Bibcode:2005ApJ...634.1093G, arXiv:astro-ph/0508251 , doi:10.1086/497023
Hopman, Clovis; Simon Portegies Zwart. Gravitational waves from remnants of ultraluminous X-ray sources. Mon.Not.Roy.Astron.Soc.Lett. 2005, 363: L56–L60. doi:10.1111/j.1745-3933.2005.00083.x.
arXiv:astro-ph/0506181
.
Schoedel, R.; A. Eckart, C. Iserlohe, R. Genzel, T. Ott. A Black Hole in the Galactic Center Complex IRS 13E?. Astrophys. J. 2005, 625: L111–L114. doi:10.1086/431307.
arXiv:astro-ph/0504474
.

Gebhardt, Karl; Rich, R. M.; Ho, Luis C., An Intermediate-Mass Black Hole in the Globular Cluster G1: Improved Significance from New Keck and Hubble Space Telescope Observations, The Astrophysical Journal, December 2005, 634 (2): 1093–1102, Bibcode:2005ApJ...634.1093G, arXiv:astro-ph/0508251 , doi:10.1086/497023
Maccarone, T.J.; et al, A black hole in a globular cluster, Nature, 2007, 455: 183–185, doi:10.1038/nature05434
Patruno, A.; Portegies Zwart, S.; Dewi, J.; Hopman, C. The ultraluminous X-ray source in M82: an intermediate-mass black hole with a giant companion. Monthly Notices of the Royal Astronomical Society: Letters. 2006, 370 (1): L6–L9 [2010-03-27]. doi:10.1111/j.1745-3933.2006.00176.x. （原始内容存档于2016-06-13）.
Hopman, Clovis; Simon Portegies Zwart. Gravitational waves from remnants of ultraluminous X-ray sources. Mon.Not.Roy.Astron.Soc.Lett. 2005, 363: L56–L60. doi:10.1111/j.1745-3933.2005.00083.x.
arXiv:astro-ph/0506181
.
Schoedel, R.; A. Eckart, C. Iserlohe, R. Genzel, T. Ott. A Black Hole in the Galactic Center Complex IRS 13E?. Astrophys. J. 2005, 625: L111–L114. doi:10.1086/431307.
arXiv:astro-ph/0504474
.

Gebhardt, Karl; Rich, R. M.; Ho, Luis C., An Intermediate-Mass Black Hole in the Globular Cluster G1: Improved Significance from New Keck and Hubble Space Telescope Observations, The Astrophysical Journal, December 2005, 634 (2): 1093–1102, Bibcode:2005ApJ...634.1093G, arXiv:astro-ph/0508251 , doi:10.1086/497023

Patruno, A.; Portegies Zwart, S.; Dewi, J.; Hopman, C. The ultraluminous X-ray source in M82: an intermediate-mass black hole with a giant companion. Monthly Notices of the Royal Astronomical Society: Letters. 2006, 370 (1): L6–L9 [2010-03-27]. doi:10.1111/j.1745-3933.2006.00176.x. （原始内容存档于2016-06-13）.

published, Robert Lea. 'Missing link' black hole found? Not so fast, new study says. Space.com. 2024-12-19 [2024-12-20] （英语）.

Black Hole Boldly Goes Where No Black Hole Has Gone Before. ESA News. January 3, 2007 [2006-05-24]. （原始内容存档于2007-01-06）.
Patruno, A.; Portegies Zwart, S.; Dewi, J.; Hopman, C. The ultraluminous X-ray source in M82: an intermediate-mass black hole with a giant companion. Monthly Notices of the Royal Astronomical Society: Letters. 2006, 370 (1): L6–L9 [2010-03-27]. doi:10.1111/j.1745-3933.2006.00176.x. （原始内容存档于2016-06-13）.
S2 and Central Black Hole. [2010-03-27]. （原始内容存档于2019-11-30）.
Dying Star Reveals More Evidence for New Kind of Black Hole | Science Blog. [2010-03-27]. （原始内容存档于2008-11-01）.