Application of a New Non-Linear Least Squares Velocity Curve Analysis Technique for Spectroscopic Binary Stars

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dc.creatorKarami, K.
dc.creatorMohebi, R.
dc.creatorSoltanzadeh, M. M.
dc.date2008-09-06
dc.date.accessioned2026-07-07T12:15:34Z
dc.date.available2026-07-07T12:15:34Z
dc.descriptionUsing measured radial velocity data of nine double lined spectroscopic binary systems NSV 223, AB And, V2082 Cyg, HS Her, V918 Her, BV Dra, BW Dra, V2357 Oph, and YZ Cas, we find corresponding orbital and spectroscopic elements via the method introduced by Karami & Mohebi (2007a) and Karami & Teimoorinia (2007). Our numerical results are in good agreement with those obtained by others using more traditional methods.
dc.description6 pages, 3 figures. Accepted for publication in Astrophysics & Space Science
dc.identifierhttps://arxiv.org/abs/0809.1175
dc.identifierhttp://arxiv.org/abs/0809.1175
dc.identifierAstrophys.SpaceSci.318:69-71,2008
dc.identifierdoi:10.1007/s10509-008-9905-5
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/211527
dc.subjectAstrophysics
dc.titleApplication of a New Non-Linear Least Squares Velocity Curve Analysis Technique for Spectroscopic Binary Stars
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