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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/343
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dc.contributor.authorJoshi, U. C-
dc.date.accessioned2005-02-09T04:13:41Z-
dc.date.available2005-02-09T04:13:41Z-
dc.date.issued1982-09-
dc.identifier.citationBASI, Vol. 10, No. 3, pp. 217-222en
dc.identifier.urihttp://hdl.handle.net/2248/343-
dc.description.abstractPlaces of formation of 10 nearby classical Cepheids have been computed in a model of our Galaxy which has axisymmetric and spiral-like components. For the axisymmetric components Schmidt's (1965) model is used, and spiral-like perturbations are approximated by logarithmic spirals. Different pattern speeds, Omega p, have been used to get the best correlation of places of formation with a spiral structure. We conclude that best fit is obtained with Omega p= 13.5 km/s kp/c.en
dc.format.extent423482 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectCepheidsen
dc.subjectdensity waveen
dc.titlePlaces of formation of nineteen nearby classical Cepheidsen
dc.typeArticleen
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