A method to deconvolve stellar rotational velocities

Aims. Rotational speed is an important physical parameter of stars, and knowing the distribution of stellar rotational velocities is essential for understanding stellar evolution. However, rotational speed cannot be measured directly and is instead the convolution between the rotational speed and th...

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Detalles Bibliográficos
Autor principal:	Rial, Diego Fernando
Publicado:	2014
Materias:	Methods:analytical Methods:data analysis Methods:numerical Methods:statistical Stars:fundamental parameters Stars:rotation Inverse problems Numerical methods Stars Velocity Velocity distribution Methods: numericals Maximum entropy methods
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v565_n_p_Cure http://hdl.handle.net/20.500.12110/paper_00046361_v565_n_p_Cure
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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