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PDS 70b Shows Stellar-like Carbon-to-oxygen Ratio

The ~5 Myr PDS 70 is the only known system with protoplanets residing in the cavity of the circumstellar disk from which they formed, ideal for studying exoplanet formation and evolution within its natal environment. Here, we report the first spin constraint and C/O measurement of PDS 70b from Keck/...

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Gespeichert in:
Hauptverfasser: Chih-Chun Hsu, Jason J. Wang, Geoffrey A. Blake, Jerry W. Xuan, Yapeng Zhang, Jean-Baptiste Ruffio, Katelyn Horstman, Julianne Cronin, Ben Sappey, Yinzi Xin, Luke Finnerty, Daniel Echeverri, Dimitri Mawet, Nemanja Jovanovic, Clarissa R. Do Ó, Ashley Baker, Randall Bartos, Benjamin Calvin, Sylvain Cetre, Jacques-Robert Delorme, Gregory W. Doppmann, Michael P. Fitzgerald, Joshua Liberman, Ronald A. López, Evan Morris, Jacklyn Pezzato-Rovner, Tobias Schofield, Andrew Skemer, J. Kent Wallace, Ji Wang
Format: Artigo
Sprache:Inglês
Veröffentlicht: IOP Publishing 2024-01-01
Schriftenreihe:The Astrophysical Journal Letters
Schlagworte:
Exoplanet atmospheres
Exoplanet formation
High resolution spectroscopy
High angular resolution
Online-Zugang:https://doi.org/10.3847/2041-8213/ad95e8
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