A method to deconvolve mass ratio distribution of binary stars

Aims. It is important to know the binary mass-ratio distribution to better understand the evolution of stars in binary systems and to constrain their formation. However, in most cases, that is, for single-lined spectroscopic binaries, the mass ratio cannot be measured directly, but can only be deriv...

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Detalles Bibliográficos
Autores principales: Curé, M., Rial, D.F., Cassetti, J., Christen, A., Boffin, H.M.J.
Formato: JOUR
Materias:
Binaries: general
Methods: analytical
Methods: data analysis
Methods: numerical
Methods: statistical
Stars: fundamental parameters
Distribution functions
Inverse problems
Stars
Systems (metallurgical)
Methods: numericals
Methods:analytical
Methods:data analysis
Methods:statistical
Stars:fundamental parameters
Numerical methods
Acceso en línea:http://hdl.handle.net/20.500.12110/paper_00046361_v573_n_p_Cure
Aporte de:
Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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