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Post-main-sequence planetary system evolution
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 dynamica...
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
The Royal Society Publishing
2016
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4785977/ https://www.ncbi.nlm.nih.gov/pubmed/26998326 http://dx.doi.org/10.1098/rsos.150571 |
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author | Veras, Dimitri |
author_facet | Veras, Dimitri |
author_sort | Veras, Dimitri |
collection | PubMed |
description | 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. |
format | Online Article Text |
id | pubmed-4785977 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2016 |
publisher | The Royal Society Publishing |
record_format | MEDLINE/PubMed |
spelling | pubmed-47859772016-03-18 Post-main-sequence planetary system evolution Veras, Dimitri R Soc Open Sci Astronomy 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. The Royal Society Publishing 2016-02-17 /pmc/articles/PMC4785977/ /pubmed/26998326 http://dx.doi.org/10.1098/rsos.150571 Text en http://creativecommons.org/licenses/by/4.0/ © 2016 The Authors. Published by the Royal Society under the terms of the Creative Commons Attribution License http://creativecommons.org/licenses/by/4.0/, which permits unrestricted use, provided the original author and source are credited. |
spellingShingle | Astronomy Veras, Dimitri Post-main-sequence planetary system evolution |
title | Post-main-sequence planetary system evolution |
title_full | Post-main-sequence planetary system evolution |
title_fullStr | Post-main-sequence planetary system evolution |
title_full_unstemmed | Post-main-sequence planetary system evolution |
title_short | Post-main-sequence planetary system evolution |
title_sort | post-main-sequence planetary system evolution |
topic | Astronomy |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4785977/ https://www.ncbi.nlm.nih.gov/pubmed/26998326 http://dx.doi.org/10.1098/rsos.150571 |
work_keys_str_mv | AT verasdimitri postmainsequenceplanetarysystemevolution |