Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2269
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dc.contributor.authorJoshi, S-
dc.contributor.authorGirish, V-
dc.contributor.authorMartinez, P-
dc.contributor.authorSagar, R-
dc.contributor.authorAshoka, B. N-
dc.contributor.authorGupta, S. K-
dc.contributor.authorSeetha, S-
dc.contributor.authorChaubey, U. S-
dc.contributor.authorKurtz, D. W-
dc.date.accessioned2008-05-07T10:14:24Z-
dc.date.available2008-05-07T10:14:24Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 3, pp. 301 - 303en
dc.identifier.urihttp://hdl.handle.net/2248/2269-
dc.description.abstractUsing the UPSO 1-m Sampurnanand reflector telescope equipped with a fast photometer, we observed the chemically peculiar (CP) star HD 98851 for a total of around 30 hours on 5 different nights between January to April 2000. From the Fourier analysis of our data we have found that HD 98851 pulsates with periods of 75.76 min and 151.52 min and amplitudes ≈ 25 mmag and 12 mmag respectively. The star appears to be a δ Scuti variable.en
dc.format.extent166344 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..301Jen
dc.subjectPulsationsen
dc.subjectHD 98851en
dc.titleDiscovery of pulsations in HD 98851en
dc.typeArticleen
Appears in Collections:BASI Publications

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