Accretion curtains in magnetic CVs

dc.contributor.author	Ferrario, Lilia	en
dc.date.accessioned	2026-01-01T15:42:06Z
dc.date.available	2026-01-01T15:42:06Z
dc.date.issued	1996	en
dc.description.abstract	We have carried out calculations to model the hydrogen emission line spectrum of intermediate polars with accretion disks. We show that we can explain most of the observed optical continuum and line fluxes in terms of hard and soft X-rays that originate from the accretion shocks and are reprocessed in curtains formed by magnetically channelled material.	en
dc.description.status	Peer-reviewed	en
dc.format.extent	6	en
dc.identifier.issn	1323-3580	en
dc.identifier.scopus	0030525325	en
dc.identifier.uri	https://hdl.handle.net/1885/733801378
dc.language.iso	en	en
dc.source	Publications of the Astronomical Society of Australia	en
dc.subject	Lines:Formation	en
dc.subject	Stars:Accretion	en
dc.subject	Stars:Binaries	en
dc.subject	Stars:Cataclysmic variables	en
dc.subject	Stars:Magnetic fields	en
dc.subject	Stars:White dwarfs	en
dc.title	Accretion curtains in magnetic CVs	en
dc.type	Journal article	en
dspace.entity.type	Publication	en
local.bibliographicCitation.lastpage	92	en
local.bibliographicCitation.startpage	87	en
local.contributor.affiliation	Ferrario, Lilia; Astrophysical Theory Centre	en
local.identifier.citationvolume	13	en
local.identifier.doi	10.1017/S1323358000020592	en
local.identifier.pure	9cd73a7e-ab63-4879-9d1d-b1b4513de515	en
local.identifier.url	https://www.scopus.com/pages/publications/0030525325	en
local.type.status	Published	en

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