Post main sequence planetary system evolution

dc.contributor.author	Veras, Dimitri	en_US
dc.date.accessioned	2016-10-11T05:37:23Z
dc.date.available	2016-10-11T05:37:23Z
dc.date.issued	2016	en_US
dc.identifier.other	HPU4160688	en_US
dc.identifier.uri	https://lib.hpu.edu.vn/handle/123456789/23580
dc.description.abstract	The 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 discoveries	en_US
dc.format.extent	65 p.	en_US
dc.format.mimetype	application/pdf
dc.language.iso	en	en_US
dc.subject	Astronomy	en_US
dc.subject	Extrasolar planets	en_US
dc.subject	Astrophysics	en_US
dc.subject	Solar system	en_US
dc.subject	Dynamics	en_US
dc.subject	White dwarfs	en_US
dc.subject	Giant branch stars	en_US
dc.subject	Pulsars	en_US
dc.subject	Asteroids	en_US
dc.subject	Formation	en_US
dc.title	Post main sequence planetary system evolution	en_US
dc.type	Article	en_US
dc.size	2.89MB	en_US
dc.department	Education	en_US