1. IIA Institutional Repository
  2. Publications of Astronomical Society of India
  3. BASI Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2410
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBabu, G. S. D-
dc.contributor.authorJayakumar, K-
dc.contributor.authorVelu, C-
dc.contributor.authorSujatha, S-
dc.date.accessioned2008-06-06T06:33:10Z-
dc.date.available2008-06-06T06:33:10Z-
dc.date.issued2003-
dc.identifier.citationBASI, Vol. 31, No. 3&4, pp. 337 - 339en
dc.identifier.urihttp://hdl.handle.net/2248/2410-
dc.description.abstractThe Sr-Cr type chemically peculiar star HD 42536 (= HR 2195) was observed with the 2.34 meter Vainu Bappu Telescope. Kavalur during the period of November 1998 to April 1999. A total of 46 spectrograms were obtained in the wavelength region of 3900 Å to 4300 Å at a linear dispersion of 0.65 Å per pixel. The equivalent widths of Sr (4077) and Cr (4172) have been found to be varying with a period of 0.58 ± 0.02 day, the amplitudes being about 100 mÅ and 60 mÅ respectively. This period is a resonance value of the peroid given by Manfroid and Mathys (1985).en
dc.format.extent85498 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2003BASI...31..337Ben
dc.subjectAp staren
dc.subjectSpectral linesen
dc.subjectVariationsen
dc.titleSpectral Line Variations in the Ap Star HD 42536en
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
paper-46.pdf83.49 kBAdobe PDFThumbnail
View/Open
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.