Long-term chromospheric activity in southern m dwarfs: Gl 229 A and Gl 752 A

Several late-type stars present activity cycles similar to that of the Sun. However, these cycles have been mostly studied in F to K stars. Due to their small intrinsic brightness, M dwarfs are not usually the targets of long-term observational studies of stellar activity, and their long-term variab...

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Detalles Bibliográficos
Autores principales:	Buccino, Andrea Paola, Díaz, Rodrigo Fernando, Luoni, Maria Luisa, Abrevaya, Ximena Celeste, Mauas, Pablo J.D.
Publicado:	2011
Materias:	Activity - stars Late-type - techniques Photometric - techniques Spectroscopic Stars
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046256_v141_n2_p_Buccino http://hdl.handle.net/20.500.12110/paper_00046256_v141_n2_p_Buccino
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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