Dynamical evolution of two planet systems into the white dwarf phase
(2019) 2019 New Quests in Stellar Astrophysics IV Astrochemistry, Astrobiology and the Origin of Life In Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society 90. p.675-677- Abstract
In this contribution we present some preliminary results on the dynamical evolution of two planet systems around stellar hosts evolving from the main sequence to the white dwarf phase. The aim is to study the instabilities triggered by stellar evolution that may bring planets onto the stellar surface or produce planetary scale collisions (hence debris) that could explain the metallic atmospheric pollution observed in white dwarfs.
Please use this url to cite or link to this publication:
https://lup.lub.lu.se/record/7b560629-b0cc-457b-b7e3-9c9dce1188e2
- author
- Maldonado, R. F. ; Villaver, E. ; Chávez, M. ; Mustill, A. LU and Bertone, E.
- organization
- publishing date
- 2019
- type
- Chapter in Book/Report/Conference proceeding
- publication status
- published
- subject
- keywords
- Stars: dynamical evolution, Stars: metal pollution, Stars: white dwarf
- host publication
- Memorie della Societa Astronomica Italiana
- series title
- Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society
- volume
- 90
- edition
- 4
- pages
- 3 pages
- conference name
- 2019 New Quests in Stellar Astrophysics IV Astrochemistry, Astrobiology and the Origin of Life
- conference location
- Puerto Vallarta, Mexico
- conference dates
- 2019-03-31 - 2019-04-05
- external identifiers
-
- scopus:85108876675
- ISSN
- 1824-016X
- language
- English
- LU publication?
- yes
- id
- 7b560629-b0cc-457b-b7e3-9c9dce1188e2
- date added to LUP
- 2021-08-16 13:00:05
- date last changed
- 2024-03-23 08:25:47
@inproceedings{7b560629-b0cc-457b-b7e3-9c9dce1188e2, abstract = {{<p>In this contribution we present some preliminary results on the dynamical evolution of two planet systems around stellar hosts evolving from the main sequence to the white dwarf phase. The aim is to study the instabilities triggered by stellar evolution that may bring planets onto the stellar surface or produce planetary scale collisions (hence debris) that could explain the metallic atmospheric pollution observed in white dwarfs.</p>}}, author = {{Maldonado, R. F. and Villaver, E. and Chávez, M. and Mustill, A. and Bertone, E.}}, booktitle = {{Memorie della Societa Astronomica Italiana}}, issn = {{1824-016X}}, keywords = {{Stars: dynamical evolution; Stars: metal pollution; Stars: white dwarf}}, language = {{eng}}, pages = {{675--677}}, series = {{Memorie della Societa Astronomica Italiana - Journal of the Italian Astronomical Society}}, title = {{Dynamical evolution of two planet systems into the white dwarf phase}}, volume = {{90}}, year = {{2019}}, }