Figure 3 from RESOLVING THE HD 100546 PROTOPLANETARY SYSTEM WITH THE GEMINI PLANET IMAGER: EVIDENCE FOR MULTIPLE FORMING, ACCRETING PLANETS

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

RESOLVING THE HD 100546 PROTOPLANETARY SYSTEM WITH THE GEMINI PLANET IMAGER: EVIDENCE FOR MULTIPLE FORMING, ACCRETING PLANETS

Authors: Thayne Currie, Ryan Cloutier, Sean Brittain, Carol Grady, Adam Burrows, Takayuki Muto, Scott J. Kenyon, and Marc J. Kuchner

2015 The Astrophysical Journal Letters 814 L27.

Provider: AAS Journals

Caption: Figure 3.

(left) PI surface brightness profile of the HD 100546 disk computed in 10° wedges as in Avenhaus et al. (2014). (right) Close-up of final IFS image showing the region around HD 100546 b and the subtraction of HD 100546 b assuming point source and 2 or 4 pixel wide extended sources. The background disk emission covers a circular region (dotted circle).

Other Images in This Article

Copyright and Terms & Conditions