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The Hubble Space Telescope Extragalactic Distance Scale Key Project. X. The Cepheid Distance to NGC 7331

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dc.contributor.author Hughes, S. M. G. en_US
dc.contributor.author Han, M. en_US
dc.contributor.author Hoessel, J. en_US
dc.contributor.author Saha, A. en_US
dc.contributor.author Silbermann, N. en_US
dc.contributor.author Stetson, P. B. en_US
dc.contributor.author Freedman, W. L. en_US
dc.contributor.author Harding, P. en_US
dc.contributor.author Kennicutt, R. C. Jr. en_US
dc.contributor.author Madore, B. F. en_US
dc.contributor.author Mould, J. R. en_US
dc.contributor.author Ferrarese, L. en_US
dc.contributor.author Ford, H. en_US
dc.contributor.author Graham, J. A. en_US
dc.contributor.author Hill, R. en_US
dc.contributor.author Huchra, J. en_US
dc.contributor.author Illingworth, G. D. en_US
dc.contributor.author Phelps, R. en_US
dc.contributor.author Sakai, S. en_US
dc.date.accessioned 2004-10-01T06:06:45Z
dc.date.available 2004-10-01T06:06:45Z
dc.date.issued 1996 en_US
dc.identifier.clearanceno 96-1653 en_US
dc.identifier.uri http://hdl.handle.net/2014/27602
dc.description.abstract The distance to NGC 7331 has been derived from Cepheid variables observed with HST/WFPC2, as part of the Extragalactic Distance Scale Key Project. Multi-epoch exposures in F555W(~V) and F814W (~1), with photometry derived independently from DoPHOT and DAOPHOT/ALLFRAME programs, which were used to detect a total of 14 reliable Cepheids, with periods between 11 and 42 days. en_US
dc.format.extent 3087614 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Cepheids galaxies distances redshifts NGC 7331 early type stars stars luminosity photometric techniques en_US
dc.title The Hubble Space Telescope Extragalactic Distance Scale Key Project. X. The Cepheid Distance to NGC 7331 en_US


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