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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2271
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dc.contributor.authorSeetha, S-
dc.contributor.authorChaubey, U. S-
dc.contributor.authorGirish, V-
dc.contributor.authorJoshi, S-
dc.contributor.authorAshoka, B. N-
dc.contributor.authorGupta, S. K-
dc.contributor.authorKurtz, D. W-
dc.contributor.authorMartinez, P-
dc.contributor.authorSagar, R-
dc.date.accessioned2008-05-07T11:34:22Z-
dc.date.available2008-05-07T11:34:22Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 309 - 312en
dc.identifier.urihttp://hdl.handle.net/2248/2271-
dc.description.abstractThe "Naini Tal-Cape survey for rapidly oscillating Ap stars", to search the northern hemi-sphere sky for pulsating stars was initiated in 1997. This is a collaboration between India and South Africa. So far about 70 stars have been observed and 4 variables have been discovered. The variables are HD 13079, HD 13038, HD 12098 and HD 98851. Of these HD 12098 is a likely rapidly oscillating Ap star. This paper gives a status report on the survey. The methodology of this survey and an evaluation of observing time vis-a-vis the chance of discovering a new variable are discussed.en
dc.format.extent280458 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..309Sen
dc.subjectNaini Tal-cape surveyen
dc.subjectPulsating starsen
dc.titleNaini Tal-Cape survey for pulsating chemically peculiar stars - A status reporten
dc.typeArticleen
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