Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

Event Horizon Telescope Pattern Speeds in the Visibility Domain

  • Authors: Nicholas S. Conroy, Michi Bauböck, Vedant Dhruv, Daeyoung Lee, Chi-kwan Chan, Abhishek V. Joshi, Cora Prather, Charles F. Gammie

Nicholas S. Conroy et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 9.

Measured (u, v) pattern speeds as a function of baseline length ρ for nearly face-on (i = 10∘, 170∘) MAD models (left) and SANE models (right), extended out past current EHT coverage. As in Figure 5, we filter out SANE Rhigh = 160, where ΩVA ≈ 0. EHT observations at 345 GHz would correspond to ρ ≲ 15Gλ, while a space VLBI mission like BHEX would extend to ρ ≈ 30Gλ.

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
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse