Figure 10 from STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

STIS Coronagraphic Imaging of Fomalhaut: Main Belt Structure and the Orbit of Fomalhaut b

Authors: Paul Kalas, James R. Graham, Michael P. Fitzgerald, and Mark Clampin

Kalas et al. 2013 The Astrophysical Journal 775 56.

Provider: AAS Journals

Caption: Figure 10.

Left panel: measurements of the peak scattered light from the main belt (red crosses) and a fit (blue crosses) based on a Keplerian orbit. Right panel: residuals between the Keplerian fit and the measured points. θ is the best-fit value of ν + ω (true anomaly + argument of perapse).

Other Images in This Article

Copyright and Terms & Conditions