Figure 8 from Probing for Exoplanets Hiding in Dusty Debris Disks: Disk Imaging, Characterization, and Exploration with HST/STIS Multi-roll Coronagraphy

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

Probing for Exoplanets Hiding in Dusty Debris Disks: Disk Imaging, Characterization, and Exploration with HST/STIS Multi-roll Coronagraphy

Authors: Glenn Schneider, Carol A. Grady, Dean C. Hines, Christopher C. Stark, John H. Debes, Joe Carson, Marc J. Kuchner, Marshall D. Perrin, Alycia J. Weinberger, John P. Wisniewski, Murray D. Silverstone, Hannah Jang-Condell, Thomas Henning, Bruce E. Woodgate, Eugene Serabyn, Amaya Moro-Martin, Motohide Tamura, Phillip M. Hinz, and Timothy J. Rodigas

Schneider et al. 2014 The Astronomical Journal 148 59.

Provider: AAS Journals

Caption: Figure 8.

Overall, debris disk-scattering fractions and thermal excesses are cross-correlated with age, but with multi-parametric dependencies, L_ir/L_star may be only a weak predictor of optical brightness for individual systems (e.g., HD 15115 in the GO 12228 sample).

Other Images in This Article

Copyright and Terms & Conditions