Bartosz Fornal et al. 2007 The Astronomical Journal 133 1409 doi:10.1086/511419
Bartosz Fornal1,2,3, Douglas L. Tucker2,4, J. Allyn Smith4,5, Sahar S. Allam2,4,6, Cristin J. Rider7 and Hwankyung Sung8
Show affiliationsWe continue our series of papers describing the results of a photometric survey of open star clusters, primarily in the southern hemisphere, taken in the u'g'r'i'z' filter system. The entire observed sample covered more than 100 clusters, but here we present data only on NGC 188, which is one of the oldest open clusters known in the Milky Way. We fit the Padova theoretical isochrones to our data. Assuming a solar metallicity for NGC 188, we find a distance of 1700 ± 100 pc, an age of 7.5 ± 0.7 Gyr, and a reddening E(B - V) of 0.025 ± 0.005. This yields a distance modulus of 11.23 ± 0.14.
Hertzsprung-Russell diagram; open clusters and associations: individual (NGC 188); stars: abundances
Issue 4 (2007 April)
Received 2006 September 1, accepted for publication 2006 November 28
Published 2007 February 26
Bartosz Fornal et al. 2007 The Astronomical Journal 133 1409
J. A. Docobo et al. 2008 The Astronomical Journal 135 1803
C K Wright et al 2009 Environ. Res. Lett. 4 045020
Warwick B Dunn 2008 Phys. Biol. 5 011001
M. Jura et al. 2007 The Astronomical Journal 133 1927
K. R. Mavani and P. L. Paulose 2007 EPL 78 37004
Carolyn Stephens 2007 Environ. Res. Lett. 2 045001
F. Lahuis et al 2006 ApJ 636 L145
M. A. Weber et al 2005 ApJ 635 L101
A S Kheifets, A Naja, E M Staicu Casagrande and A Lahmam-Bennani 2008 J. Phys. B: At. Mol. Opt. Phys. 41 209801