A Survey of Open Clusters in the u'g'r'i'z' Filter System: III. Results for the Cluster NGC 188

dc.creatorFornal, Bartosz
dc.creatorTucker, Douglas L.
dc.creatorSmith, J. Allyn
dc.creatorAllam, Sahar S.
dc.creatorRider, Cristin J.
dc.creatorSung, Hwankyung
dc.date2006-11-29
dc.date.accessioned2026-07-07T11:20:47Z
dc.date.available2026-07-07T11:20:47Z
dc.descriptionWe 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.
dc.description41 pages, 8 figures. Accepted for publication in the Astronomical Journal
dc.identifierhttps://arxiv.org/abs/astro-ph/0611900
dc.identifierhttp://arxiv.org/abs/astro-ph/0611900
dc.identifierAstron.J.133:1409-1420,2007
dc.identifierdoi:10.1086/511419
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/194066
dc.subjectAstrophysics
dc.titleA Survey of Open Clusters in the u'g'r'i'z' Filter System: III. Results for the Cluster NGC 188
dc.typetext

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