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A Carbon-rich Atmosphere on a Windy Pulsar Planet

A handful of enigmatic Jupiter-mass objects have been discovered orbiting pulsars. One such object, PSR J2322–2650b, uniquely resembles a hot-Jupiter exoplanet, due to its minimum density of 1.8 g cm ^−3 and its ∼1900 K equilibrium temperature. We use JWST to observe PSR J2322–2650b’s emission spect...

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Autors principals: Michael Zhang, Maya Beleznay, Timothy D. Brandt, Roger W. Romani, Peter Gao, Hayley Beltz, Matthew Bailes, Matthew C. Nixon, Jacob L. Bean, Thaddeus D. Komacek, Brandon P. Coy, Guangwei Fu, Rafael Luque, Daniel J. Reardon, Emma Carli, Ryan M. Shannon, Jonathan J. Fortney, Anjali A. A. Piette, M. Coleman Miller, Jean-Michel Desert
Format: Artigo
Idioma:Inglês
Publicat: IOP Publishing 2025-01-01
Col·lecció:The Astrophysical Journal Letters
Matèries:
Pulsar planets
Carbon planets
Hot Jupiters
High energy astrophysics
Stellar atmospheres
Accés en línia:https://doi.org/10.3847/2041-8213/ae157c
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