Origin of magnetism in early-type stars

De acuerdo a nuestro entendimiento de la evolución estelar, las estrellas de tipo temprano poseen envolturas radiativas y núcleos convectivos debido a un fuerte gradiente de temperatura producido por el ciclo CNO. Algunas de estas estrellas (principalmente, las subclases Ap y Bp) tienen fuertes camp...

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Detalles Bibliográficos
Autores principales:	Hidalgo, Juan Pablo, Käpylä, Petri, Ortiz Rodríguez, Carolina Angélica, Navarrete, Felipe, Toro, Bárbara, Schleicher, Dominik
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2023
Materias:	Ciencias Astronómicas stars: magnetic field stars: massive magnetohydrodynamics (MHD) dynamo
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/164172
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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