Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7505
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dc.contributor.authorGurumath, S. R-
dc.date.accessioned2019-08-08T08:37:14Z-
dc.date.available2019-08-08T08:37:14Z-
dc.date.issued2019-05-
dc.identifier.citationPh.D. Thesis, Vellore Institute of Technology ,Velloreen_US
dc.identifier.urihttp://hdl.handle.net/2248/7505-
dc.descriptionThesis Supervisors Prof. V. Ramasubramanian and Prof K. M. Hiremathen_US
dc.description.abstractBy employing exoplanetary physical and orbital characteristics, aim of this study is to understand the genesis, dynamics, chemical abundance and magnetic field structure of Sun-like G stars and relationship with their planets. With reasonable constraints on selection of exoplanetary physical characteristics, and by making corrections for stellar rate of mass loss, a power law relationship between initial stellar mass and their exoplanetary mass is obtained that suggests massive stars harbor massive planets.en_US
dc.language.isoenen_US
dc.publisherVellore Institute of Technology and Indian Institute of Astrophysicsen_US
dc.subjectExoplanetsen_US
dc.subjectSunen_US
dc.subjectSolar systemen_US
dc.subjectstars:evolutionen_US
dc.titleStudy of sun-like G stars and their exoplanetsen_US
dc.typeThesisen_US
Appears in Collections:IIAP Ph.D.Theses

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