Search for P-mode pulsctions in late-type CP Stars

dc.contributor.author	Joshi, S.
dc.contributor.author	Chakradhari, S. Joshi
dc.date.accessioned	2013-05-21T05:07:25Z
dc.date.available	2013-05-21T05:07:25Z
dc.date.issued	2011
dc.identifier.uri	http://hdl.handle.net/123456789/925
dc.description.abstract	The Sun, solar-like oscillators, δ-Scuti and roAp stars are few examples of the main-sequence pulsating stars for which the quantitative measurements of the internal structure parameters have been derived from their oscillations. For the asteroseismic study of δ-Sct and roAp stars, a project the “Nainital-Cape Survey” is being run at ARIES, Nainital since 1999. In this paper, we present the overview of stellar-seismology and briefly describe the results obtained under the survey project.	en_US
dc.language.iso	en_US	en_US
dc.publisher	Adv. Geo.	en_US
dc.relation.ispartofseries	advgeo-27-219
dc.subject	Sun, Solar System	en_US
dc.title	Search for P-mode pulsctions in late-type CP Stars	en_US
dc.type	Article	en_US