Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

The HD 60779 Planetary System: A Transiting Sub-Neptune on a 30 Day Orbit and a More Massive Outer World

  • Authors: Victoria DiTomasso, David Charbonneau, Andrew Vanderburg, Mercedes López- Morales, Shreyas Vissapragada, Annelies Mortier, Thomas G. Wilson, Elyse Incha, Andrew Collier Cameron, Luca Malavolta, Lars A. Buchhave, David W. Latham, Matteo Pinamonti, Stephanie Striegel, Michael Fausnaugh, Luke Bouma, Ben Falk, Robert Aloisi, Xavier Dumusque, A. Anna John, Ben S. Lakeland, A. F. Martínez Fiorenzano, Luca Naponiello, Belinda Nicholson, Emily K. Pass, Francesco Alfonso Pepe, Federica Rescigno, Alessandro Sozzetti, Daisy A. Turner, Saul A. Rappaport, Mark Omohundro, Brian P. Powell, Robert Gagliano, Thomas L. Jacobs, Veselin B. Kostov, Martti H. Kristiansen, Daryll M. LaCourse, Allan R. Schmitt, Hans Martin Schwengeler, Ivan A. Terentev

Victoria DiTomasso et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 7.

Final RV and transit fits. The left and center panels show the phase-folded RV curves for HD 60779 b and HD 60779 c, respectively. The right panel shows the phase-folded transit light curves from TESS Sectors 34 and 88, and from CHEOPS. The red points in all panels show binned values. The stated eccentricities are the 1σ upper limits.

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

Show More

Copyright and Terms & Conditions

Additional terms of reuse