Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society, 3(441), p. 2380-2391, 2014
DOI: 10.1093/mnras/stu721
Links
Tools
Planetesimal-driven migration as an explanation for observations of high levels of warm, exozodiacal dust
This paper was not found in any repository, but could be made available legally by the author.
Full text: Unavailable
Data provided by 
