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20242026
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astro-ph.EP2026

Asymmetric, variable H line profile in planetary mass object SR 12 c

Jun Hashimoto, Yuhiko Aoyama, Michihiro Takami +1

Young, forming planetary-mass objects often exhibit clear signatures of ongoing mass accretion and are thought to accrete material through processes analogous to those operating in…

astro-ph.EP2025

Characterizing the Time Variability of 2M1207 A+b with JWST NIRSpec/PRISM

Arthur D. Adams, Yifan Zhou, Gabriel Dominique-Marleau +13

We present JWST NIRSpec/PRISM IFU time-resolved observations of 2M1207 A and b (TWA 27), a Myr binary system consisting of a K sub-stellar primary hosting a $…

astro-ph.EP2025

Evidence for Variable Accretion onto PDS 70 c and Implications for Protoplanet Detections

Yifan Zhou, Brendan P. Bowler, Aniket Sanghi +14

Understanding the processes of planet formation and accretion in young systems is essential to unraveling the initial conditions of planetary systems. The PDS 70 system, which host…

astro-ph.EP2024

Analyses of Multiple Balmer Emission Lines from Accreting Brown Dwarfs and Very Low Mass Stars

Jun Hashimoto, Yuhiko Aoyama

A planetary growth rate, a.k.a., the mass accretion rate, is a fundamental parameter in planet formation, as it determines a planet's final mass. Planetary mass accretion rates hav…

astro-ph.EP2024

Analyzing JWST/NIRSpec Hydrogen Line Detections at TWA 27B: Constraining Accretion Properties and Geometry

Yuhiko Aoyama, Gabriel-Dominique Marleau, Jun Hashimoto

Hydrogen lines from forming planets are crucial for understanding planet formation. However, the number of planetary hydrogen line detections is still limited. Recent JWST/NIRSpec…