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Please use this identifier to cite or link to this item: https://lib.hpu.edu.vn/handle/123456789/23580
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dc.contributor.authorVeras, Dimitrien_US
dc.date.accessioned2016-10-11T05:37:23Z
dc.date.available2016-10-11T05:37:23Z
dc.date.issued2016en_US
dc.identifier.otherHPU4160688en_US
dc.identifier.urihttps://lib.hpu.edu.vn/handle/123456789/23580-
dc.description.abstractThe fates of planetary systems provide unassailable insights into their formation and represent rich cross-disciplinary dynamical laboratories. Mounting observations of post-main-sequence planetary systems necessitate a complementary level of theoretical scrutiny. Here, I review the diverse dynamical processes which affect planets, asteroids, comets and pebbles as their parent stars evolve into giant branch, white dwarf and neutron stars. This reference provides a foundation for the interpretation and modelling of currently known systems and upcoming discoveriesen_US
dc.format.extent65 p.en_US
dc.format.mimetypeapplication/pdf-
dc.language.isoenen_US
dc.subjectAstronomyen_US
dc.subjectExtrasolar planetsen_US
dc.subjectAstrophysicsen_US
dc.subjectSolar systemen_US
dc.subjectDynamicsen_US
dc.subjectWhite dwarfsen_US
dc.subjectGiant branch starsen_US
dc.subjectPulsarsen_US
dc.subjectAsteroidsen_US
dc.subjectFormationen_US
dc.titlePost main sequence planetary system evolutionen_US
dc.typeArticleen_US
dc.size2.89MBen_US
dc.departmentEducationen_US
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