Ultraviolet Imaging of SR 12 c with HST/WFC3: Accretion and Variability of a Giant Planet at the End Stages of Growth
Claire O. Finley, Brendan P. Bowler, Ya-Lin Wu, Adam L. Kraus, Yifan Zhou, Yuhiko Aoyama, William Best, Ian Czekala, Catherine C. Espaillat, Katherine B. Follette, Gregory J. Herczeg, Raquel A. Martinez, Connor E. Robinson, Quang H. Tran, Kimberly Ward-Duong
astro-ph.EP
Submitted: 2026-06-11
Comments: Accepted for publication in AJ
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Spectral appearance of the planetary-surface accretion shock: Global spectra and hydrogen-line profiles and fluxes
- Evolutionary models for solar metallicity low-mass stars: mass-magnitude relationships and color-magnitude diagrams
- Optical and Near-infrared View of Planet-forming Disks and Protoplanets
- H$\alpha$ Variability of AB Aur b with the Hubble Space Telescope: Probing the Nature of a Protoplanet Candidate with Accretion Light Echoes
- The Pan-STARRS1 Surveys
- A carbon-rich disk surrounding a planetary-mass companion
- Gravitational Instabilities in Gaseous Protoplanetary Disks and Implications for Giant Planet Formation
- The Origin and Evolution of Multiple Star Systems
- JWST/MIRI observations of the young TWA 27 system: hydrocarbon disk chemistry, silicate clouds, evidence for a CPD
- Star Formation in the rho Ophiuchi Molecular Cloud
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