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Modelling the variability of the Fe Kα line in accreting black holes |
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| Authors: | Piotr T &#;ycki |
| Institution: | Dpto. de Física, Facultad de Ciencias Físicas y Matemáticas, Universidad de Concepción, Casilla 160-C, Concepción, Chile;Instituto Astronômico e Geofísico, Universidade de São Paulo, Brazil |
| Abstract: | |
| Keywords: | binaries: close stars: dwarf novae stars: evolution stars: fundamental parameters stars: low-mass brown dwarfs novae cataclysmic variables |