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Properties of Magnetic Accretion Curtains: Magnetic CVs and T Tauri Stars

Published online by Cambridge University Press:  12 April 2016

Lilia Ferrario
Lilia Ferrario*
Affiliation:
Department of Mathematics & the Astrophysical Theory Centre, The Australian National University, Canberra, ACT 0200, Australia.

Abstract

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In this paper, I present a review on the properties of accretion curtains in magnetic Cataclysmic Variables and T Tauri stars. In particular, I will show that magnetically confined accretion curtains that are heated by hard, soft x-rays or UV radiation originating from the accretion shocks at the surface of the accreting star can give rise to the observed complex emission line profiles.

Type
Part 9. Accretion Curtains and Funnels
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 403 - 408
Copyright
Copyright © Astronomical Society of the Pacific 1997

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