Places of formation of nineteen nearby classical Cepheids

dc.contributor.author	Joshi, U. C
dc.date.accessioned	2005-02-09T04:13:41Z
dc.date.available	2005-02-09T04:13:41Z
dc.date.issued	1982-09
dc.identifier.citation	BASI, Vol. 10, No. 3, pp. 217-222	en
dc.identifier.uri	http://hdl.handle.net/2248/343
dc.description.abstract	Places 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.extent	423482 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	Cepheids	en
dc.subject	density wave	en
dc.title	Places of formation of nineteen nearby classical Cepheids	en
dc.type	Article	en