Star-Planet Interaction at radio wavelengths in YZ Ceti: Inferring planetary magnetic field

In exoplanetary systems, the interaction between the central star and the planet can trigger Auroral Radio Emission (ARE), due to the Electron Cyclotron Maser mechanism. The high brightness temperature of this emission makes it visible at large distances, opening new opportunities to study exoplanet...

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Veröffentlicht in:	arXiv.org 2023-05
Hauptverfasser:	Trigilio, Corrado, Biswas, Ayan, Leto, Paolo, Umana, Grazia, Busa, Innocenza, Cavallaro, Francesco, Das, Barnali, Chandra, Poonam, Perez-Torres, Miguel, Wade, Gregg A, Bordiu, Cristobal, Buemi, Carla S, Bufano, Filomena, Ingallinera, Adriano, Loru, Sara, Riggi, Simone
Format:	Artikel
Sprache:	eng
Schlagworte:	Brightness temperature Circular polarization Cyclotrons Emission analysis Extrasolar planets M stars Magnetic fields Magnetospheres Planetary atmospheres Planetary evolution Planetary magnetic fields Planetary systems Radio astronomy Radio emission Radio telescopes Wavelengths
Online-Zugang:	Volltext
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