Omega Centauri (Dutch Wikipedia)

Analysis of information sources in references of the Wikipedia article "Omega Centauri" in Dutch language version.

refsWebsite

Global rank Dutch rank

18^th place

273^rd place

2^nd place

8^th place

1^st place

doi.org

Noyola, E. and Gebhardt, K. and Bergmann, M. (apr 2008). Gemini and Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in ω Centauri. The Astrophysical Journal 676: 1008–1015. DOI: 10.1086/529002. arxiv|0801.2782
Anderson, J. and van der Marel, R. P. (feb 2010). New Limits on an Intermediate-Mass Black Hole in Omega Centauri. I. Hubble Space Telescope Photometry and Proper Motions. The Astrophysical Journal 710: 1032–1062. DOI: 10.1088/0004-637X/710/2/1032. arxiv|0905.0627
van der Marel, R.P. and Anderson, J. (feb 2010). New Limits on an Intermediate-Mass Black Hole in Omega Centauri. II. Dynamical Models. The Astrophysical Journal 710: 1063–1088. DOI: 10.1088/0004-637X/710/2/1063. arxiv|0905.0638
van de Ven, G.; van den Bosch, R.C.E.; Verolme, E.K.; de Zeeuw, P.T. (January II 2006). The dynamical distance and intrinsic structure of the globular cluster ω Centauri. Astronomy and Astrophysics 445 (2): 513–543. DOI: 10.1051/0004-6361:20053061. “best-fit dynamical distance D = 4,8 ± 0,3 kpc ... consistent met de klassieke waarde van 5,0 ± 0,2 kpc bepaald met fotometrie”.

Noyola, E. and Gebhardt, K. and Bergmann, M. (apr 2008). Gemini and Hubble Space Telescope Evidence for an Intermediate-Mass Black Hole in ω Centauri. The Astrophysical Journal 676: 1008–1015. DOI: 10.1086/529002. arxiv|0801.2782
Anderson, J. and van der Marel, R. P. (feb 2010). New Limits on an Intermediate-Mass Black Hole in Omega Centauri. I. Hubble Space Telescope Photometry and Proper Motions. The Astrophysical Journal 710: 1032–1062. DOI: 10.1088/0004-637X/710/2/1032. arxiv|0905.0627
van der Marel, R.P. and Anderson, J. (feb 2010). New Limits on an Intermediate-Mass Black Hole in Omega Centauri. II. Dynamical Models. The Astrophysical Journal 710: 1063–1088. DOI: 10.1088/0004-637X/710/2/1063. arxiv|0905.0638
van de Ven, G.; van den Bosch, R.C.E.; Verolme, E.K.; de Zeeuw, P.T. (January II 2006). The dynamical distance and intrinsic structure of the globular cluster ω Centauri. Astronomy and Astrophysics 445 (2): 513–543. DOI: 10.1051/0004-6361:20053061. “best-fit dynamical distance D = 4,8 ± 0,3 kpc ... consistent met de klassieke waarde van 5,0 ± 0,2 kpc bepaald met fotometrie”.