Planetesimal-driven migration as an explanation for observations of high levels of warm, exozodiacal dust (2014)
Attributed to:
Research in planetary formation, astrophysics, and cosmology at Bristol
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1093/mnras/stu721
Publication URI: http://dx.doi.org/10.1093/mnras/stu721
Type: Journal Article/Review
Parent Publication: Monthly Notices of the Royal Astronomical Society
Issue: 3