G. van de Ven, R.C.E. van den Bosch, E.K. Verolme, P.T. de Zeeuw. The dynamical distance and intrinsic structure of the globular cluster ω Centauri. „Astronomy and Astrophysics”. 445 (2), s. 513–543, 2 stycznia 2006. DOI: 10.1051/0004-6361:20053061. arXiv:astro-ph/0509228. Bibcode: 2006A&A...445..513V. Cytat: best-fit dynamical distance D=4.8±0.3 kpc ... consistent with the canonical value 5.0±0.2 kpc obtained by photometric methods. (ang.).
G. van de Ven, R.C.E. van den Bosch, E.K. Verolme, P.T. de Zeeuw. The dynamical distance and intrinsic structure of the globular cluster ω Centauri. „Astronomy and Astrophysics”. 445 (2), s. 513–543, 2 stycznia 2006. DOI: 10.1051/0004-6361:20053061. arXiv:astro-ph/0509228. Bibcode: 2006A&A...445..513V. Cytat: best-fit dynamical distance D=4.8±0.3 kpc ... consistent with the canonical value 5.0±0.2 kpc obtained by photometric methods. (ang.).
G. van de Ven, R.C.E. van den Bosch, E.K. Verolme, P.T. de Zeeuw. The dynamical distance and intrinsic structure of the globular cluster ω Centauri. „Astronomy and Astrophysics”. 445 (2), s. 513–543, 2 stycznia 2006. DOI: 10.1051/0004-6361:20053061. arXiv:astro-ph/0509228. Bibcode: 2006A&A...445..513V. Cytat: best-fit dynamical distance D=4.8±0.3 kpc ... consistent with the canonical value 5.0±0.2 kpc obtained by photometric methods. (ang.).