Time-resolved spectroscopy of the AM Herculis-type binary systems QQ VUL and EF ERI

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dc.contributor.advisor Kaitchuck, Ronald H. en_US
dc.contributor.author Blakelock, Carolyn J. en_US
dc.date.accessioned 2011-06-03T19:38:11Z
dc.date.available 2011-06-03T19:38:11Z
dc.date.created 1998 en_US
dc.date.issued 1998
dc.identifier LD2489.Z78 1998 .B57 en_US
dc.identifier.uri http://cardinalscholar.bsu.edu/handle/handle/186131
dc.description.abstract Cataclysmic variable stars (CVs) are interacting binary systems. One of the stars (referred to as the primary) is a white dwarf, the other (referred to as the secondary) is usually a late main sequence star such as a red dwarf. Due to the closeness of the two stars, the white dwarf accretes gasses from the secondary. If the white dwarf does not possess a strong magnetic field, these gasses go into orbit, forming an accretion disk around the primary. If the white dwarf does possess a strong magnetic field, the gasses cannot form an accretion disk because they are entrained by the magnetic field lines. Cataclysmic variable stars in which the magnetic field is strong enough to prevent the formation of the accretion disk are called AM Herculis-type systems, after their prototype. In this study, the time-resolved spectroscopy of two AM Herculis-type binary systems, QQ Vul and EF Eri, are analyzed. In addition, Doppler Tomography, an analysis technique previously applied primarily to cataclysmic variable stars with accretion disks, is applied to these systems.
dc.description.sponsorship Department of Physics and Astronomy
dc.format.extent v, 69 leaves : ill. ; 28 cm. en_US
dc.source Virtual Press en_US
dc.subject.lcsh Cataclysmic variable stars. en_US
dc.subject.lcsh Accretion (Astrophysics) en_US
dc.subject.lcsh Dwarf stars. en_US
dc.subject.lcsh Magnetohydrodynamics. en_US
dc.title Time-resolved spectroscopy of the AM Herculis-type binary systems QQ VUL and EF ERI en_US
dc.description.degree Thesis (M.S.)
dc.identifier.cardcat-url http://liblink.bsu.edu/catkey/1115429 en_US


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  • Master's Theses [5454]
    Master's theses submitted to the Graduate School by Ball State University master's degree candidates in partial fulfillment of degree requirements.

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