Bombardment Models of White Dwarf Accretion Columns

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Scientific paper

The problem of the observed low ratio of hard to soft X-rays in
accreting white dwarfs, with low accretion rates, (e.g. AM Her) is
discussed in terms of models where the accreting matter is treated as a
non-thermal stream bombarding a static atmosphere cooled by optically
thin radiation (Kuijpers & Pringle, 1982).

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