INVESTIGADORES
MAUAS Pablo Jacobo David
congresos y reuniones científicas
Título:
Actividad cromosférica en estrellas frías
Autor/es:
IBAÑEZ BUSTOS, R.; FLORES, M.; BUCCINO, A.P.; MAUAS, P. J. D.
Lugar:
San Juan
Reunión:
Congreso; Reunion anual de la Asociación Argentina de Astronomía; 2016
Institución organizadora:
Asociación Argentina de Astronomía
Resumen:
The magnetic fields that cause stellar activity, are generated by theinteraction between the convection and stellar rotation (stellardynamo). In cooler stars, convection becomes dominant. It has beenreported that late-type dM stars, even the purely convective ones,present higher levels of activity than those found for the earlieststars. In this article, we present the mean level of activity andvariability of a set of eight dM stars from the observations obtainedunder the HK Project, which operates in the Complejo AstronómicoEl Leoncito (CASLEO) since 1999.
