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/2248/621
Full metadata record
DC FieldValueLanguage
dc.contributor.authorRadhakrishnan, K. R-
dc.contributor.authorAbhyankar, K. D-
dc.contributor.authorSarma, M. B. K-
dc.date.accessioned2005-12-06T09:50:20Z-
dc.date.available2005-12-06T09:50:20Z-
dc.date.issued1984-06-
dc.identifier.citationBASI, Vol. 12, No. 2, pp. 182-189en
dc.identifier.urihttp://hdl.handle.net/2248/621-
dc.description.abstractPhotoelectric observations of the Algol-type eclipsing binary R Canis Majoris during three consequtive observing seasons of 1979-82 gave a total of ten primary minima in each of the V and B passbands and nine in the U passband. The (O - C) curve obtained by using these minima and those available in the literature indicates that the period changes noticed in R CMa are due to light-time effect. The elements of the light-time orbit are determined. The mass of the third body is derived to be ~~ 0.5 M for i values ranging from 60/supo/ to 90/supo/. The low mass and the absence of significant light contribution suggests that the third body may me an M dwarf or a white dwarf.en
dc.format.extent616246 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectEclipsing Binaryen
dc.subjectR CMaen
dc.subjectTriple systemen
dc.titlePeriod study of the Algol-type eclipsing binary - R Canis Majorisen
dc.typeArticleen
Appears in Collections:BASI Publications

Files in This Item:
File Description SizeFormat 
RADHAKRISHNAN.pdf601.8 kBAdobe PDFThumbnail
View/Open
Show simple item record


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