Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Occurrence Rates of Accreting Companions from a New Method for Computing Emission-line Survey Sensitivity: Application to the Hα Giant Accreting Protoplanet Survey

  • Authors: Cailin Plunkett, Katherine B. Follette, Gabriel-Dominique Marleau, Eric L. Nielsen

Cailin Plunkett et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 4.

Survey-averaged completeness to accreting companions as a function of projected separation (mas) and ﹩M\dot{M}﹩ (﹩{M}_{{\rm{J}}}^{2}\,{\mathrm{yr}}^{-1}﹩ ). The five GAPlanetS detections are overplotted as white stars. From upper left to lower right, these are CS Cha c, LkCa 15 b, HD 142527 B, PDS 70 c, and HD 100453 B.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse