Places of formation of nineteen nearby classical Cepheild

dc.contributor.author	Joshi, U. C.
dc.date.accessioned	2010-04-22T06:10:42Z
dc.date.available	2010-04-22T06:10:42Z
dc.date.issued	1982
dc.identifier.uri	http://hdl.handle.net/123456789/663
dc.description.abstract	Places of formation of 19 nearby classical Cepheids have been computed in a model of our Galaxy which has axisymmetric and spiral-like components. For the axisymmetric component Schmidt’s (1965) model is used, and spsiral-like perturbations are approximated by logarithmic spirals. Different pattern speeds, Ωp, have been used to get the best correlation of places of formation with a spiral structure. We conclude that best fit is obtained with Ωp = 13.5 km s-¹ kpc-¹.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi10-217
dc.subject	Cepheids, Density Wave	en_US
dc.title	Places of formation of nineteen nearby classical Cepheild	en_US
dc.type	Article	en_US