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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2732
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dc.contributor.authorSeetha, S-
dc.contributor.authorAshoka, B. N-
dc.contributor.authorJoshi, S-
dc.contributor.authorGirish, V-
dc.contributor.authorSagar, R-
dc.contributor.authorChaubey, U. S-
dc.contributor.authorGupta, S. K-
dc.date.accessioned2008-07-17T12:08:53Z-
dc.date.available2008-07-17T12:08:53Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 623 - 629en
dc.identifier.urihttp://hdl.handle.net/2248/2732-
dc.description.abstractThe Naini Tal-Cape survey has been initiated to search for pulsations in chemically peculiar A and F type stars. Many of the magnetic A peculiar type stars exhibit rapid oscillations with periods ranging from 4-16 minutes. These stars are termed as rapidly oscillating Ap stars (roAp) stars. The oscillations are attributed to low order, high overtone p modes. In addition to the Ap stars, this region of the HR diagram also encompasses the non-magnetic 'Am' or metallic lined stars. Some of these Am stars exhibit low overtone 6 Scuti type pulsations. The scientific motivation for a study of these oscillations is discussed along with the results on the variables discovered from the survey.en
dc.format.extent223841 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectroAP-CP-pulsations-starsen
dc.subjectHD 12098 13038-HD 13079-HD 98851en
dc.titleNew pulsating variables discovered from the Naini Tal-Cape surveyen
dc.typeArticleen
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