The Modeling of the Physical and Dynamical Properties of Spectroscopic Binaries with an Orbit

This memory, devoted on Spectroscopic Binaries (SBs), was realizad by Ahmad Ali Marzouq Abushattal at the Ramon Maria Aller Astronomical Observatory (OARMA) of the University of Santiago de Compostela (Galicia, Spain), and was proposed and directed by Professor Jose Angel Docobo. The main body of th...

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Detalles Bibliográficos
Autor: Marzouq Abushattal, Ahmad Ali
Tipo de recurso: tesis doctoral
Fecha de publicación:2017
País:España
Institución:Universidad de Santiago de Compostela (USC)
Repositorio:Minerva. Repositorio Institucional de la Universidad de Santiago de Compostela
Idioma:inglés
OAI Identifier:oai:minerva.usc.gal:10347/15692
Acceso en línea:http://hdl.handle.net/10347/15692
Access Level:acceso abierto
Palabra clave:Materias::Investigación::21 Astronomía Astrofísica::2101 Cosmología y cosmogonía::210101 Estrellas dobles
Descripción
Sumario:This memory, devoted on Spectroscopic Binaries (SBs), was realizad by Ahmad Ali Marzouq Abushattal at the Ramon Maria Aller Astronomical Observatory (OARMA) of the University of Santiago de Compostela (Galicia, Spain), and was proposed and directed by Professor Jose Angel Docobo. The main body of the dissertation corresponds to obtaining the diferent steps necessary to describe the most probable 3-dimensional model of the spectroscopic binaries, especially their apparent orbits, which permit to us to have an idea about their separations in order to try to resolve them optically with the adequate telescope. The methodology (programmed in MATLAB) is applied to 25 real cases as well as the testing with 5 SBs prevously resolved by means of speckle interferometry.

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