Document Type
Article
Publication Date
2-13-2020
Publication Title
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press
Volume
494
Issue
1
First page number:
L17
Last page number:
L21
Abstract
Polluted white dwarfs are generally accreting terrestrial-like material that may originate from a debris belt like the asteroid belt in the Solar system. ... See full text for complete abstract.
Keywords
Minor Planets; Asteroids: general; Planets and satellites: dynamical evolution and stability; Stars: AGB and post-AGB; White dwarfs
Disciplines
External Galaxies | Physical Processes | Stars, Interstellar Medium and the Galaxy
File Format
File Size
339 KB
Language
English
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.
Repository Citation
Martin, R. G.,
Livio, M.,
Smallwood, J. L.,
Chen, C.
(2020).
Asteroid Belt Survival through Stellar Evolution: Dependence on the Stellar Mass.
Monthly Notices of the Royal Astronomical Society, 494(1),
L17-L21.
Oxford University Press.
http://dx.doi.org/10.1093/mnrasl/slaa030
Included in
External Galaxies Commons, Physical Processes Commons, Stars, Interstellar Medium and the Galaxy Commons
