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Worlds in Migration

Lund, Michael B. (2019) Worlds in Migration. . (Unpublished) http://resolver.caltech.edu/CaltechAUTHORS:20190520-090948164

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Abstract

In this paper we discuss an alternative track for migration that can explain the existence of Hot Jupiters observed in close orbits around their stars based on a novel interpretation of established work. We also discuss the population of sub-Earth rogue planets that would be created via this migration method, which would be on the order of 2 to 40 billion, many of which would still be present in the Galaxy and potentially detectable.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
https://arxiv.org/abs/1903.12437arXivDiscussion Paper
ORCID:
AuthorORCID
Lund, Michael B.0000-0003-2527-1598
Additional Information:The author thanks Savannah R. Jacklin for her valuable feedback on this manuscript. This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al., 2013; Price-Whelan et al., 2018).
Group:Infrared Processing and Analysis Center (IPAC)
Record Number:CaltechAUTHORS:20190520-090948164
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190520-090948164
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:95589
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:20 May 2019 17:24
Last Modified:20 May 2019 17:24

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