A Bayesian Analysis of Models for the Dust Cloud around Fomalhaut
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/538/i=2/a=783/pdf
Reference11 articles.
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2. Infrared observations and thermal models of the Beta Pictoris disk
3. Backman, D. E. & Parsece, F. 1993, in Protostars and Planets III, ed. E. H. Levy & J. I. Lunine (Tuscon: Univ. of Arizona Press), 1253
4. Gillett, F. C. 1986, Light on Dark Matter, ed. F. Israel (Dordrecht: Reidel), 61
5. Far‐Infrared Constraints on Dust Shells around Vega‐Like Stars
Cited by 3 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献
1. Dusty Debris Disks as Signposts of Planets: Implications forSpitzer Space Telescope;The Astrophysical Journal;2004-03-10
2. Collisional processes in extrasolar planetesimal discs - dust clumps in Fomalhaut's debris disc;Monthly Notices of the Royal Astronomical Society;2002-08-11
3. Dusty Circumstellar Disks;Annual Review of Astronomy and Astrophysics;2001-09
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