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
Autores principales: Curé, M., Rial, D.F., Christen, A., Cassetti, J.
Formato: JOUR
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: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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