First detection of variable radio emission originating from the infant planetary system V1298 Tau

Context. V1298 Tau is a very young and magnetically active K1V star that hosts a benchmark multi-planetary system to study planet formation and evolutionary history at the earliest stages. Thanks to the high interest, it has been the target of a multi-wavelength follow-up.

Detalles Bibliográficos
Autores: Damasso, M., Morata, Óscar, Kaur, S., Viganò, Daniele, Melis, A., Murgia, M., Pilia, Maura, Lanza, A., Del Sordo, Fabio, Antonietti, N., Kansabanik, Devojyoti, Molinari, E., Pérez-Torres, Miguel A., Sánchez-Monge, Álvaro, Maggio, A., Girart, Josep Miquel
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2025
País:España
Institución:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/389560
Acceso en línea:http://hdl.handle.net/10261/389560
Access Level:acceso abierto
Palabra clave:Planet-star interactions
Planetary systems
Stars: individual: V1298Tau
Radio continuum: planetary systems
Radio continuum: stars
Descripción
Sumario:Context. V1298 Tau is a very young and magnetically active K1V star that hosts a benchmark multi-planetary system to study planet formation and evolutionary history at the earliest stages. Thanks to the high interest, it has been the target of a multi-wavelength follow-up.

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