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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4195
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dc.contributor.authorAshoka, B. N-
dc.contributor.authorSurendiranath, R-
dc.contributor.authorKameswara Rao, N-
dc.date.accessioned2008-12-29T14:17:13Z-
dc.date.available2008-12-29T14:17:13Z-
dc.date.issued1985-
dc.identifier.citationActa Astronomica, Vol. 35, No. 3 - 4, pp. 395 - 399en
dc.identifier.issn0001-5237-
dc.identifier.urihttp://hdl.handle.net/2248/4195-
dc.description.abstractPresented are radial-velocity observations of the single-line spectroscopic binary and Beta Cephei-type variable Nu Cen, obtained in the period 1983-1984. New orbital elements have been determined by combining these observations with observations obtained 80 years earlier. In addition to the orbital period, Beta Cephei-type variability with 0.1690156-day periodicity seems to be present in these observations.en
dc.language.isoenen
dc.publisherCopernicus Foundation for Polish Astronomyen
dc.relation.urihttp://adsabs.harvard.edu/abs/1985AcA....35..395Aen
dc.subjectBinary Starsen
dc.subjectCepheid Variablesen
dc.subjectLine Spectraen
dc.subjectRadial Velocityen
dc.subjectStellar Spectrophotometryen
dc.subjectOrbital Elementsen
dc.subjectVelocity Measurementen
dc.titleSpectroscopic observations of Nu Centaurien
dc.typeArticleen
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