The shape of the Fe K alfa spectral line in the case of partly obscured accretion disk

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The shape of the Fe K alfa spectral line in the case of partly obscured accretion disk

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dc.contributor.author Jovanović, Predrag
dc.contributor.author Popović, Luka Č.
dc.contributor.editor Popović, Luka Č.
dc.date.accessioned 2011-01-14T10:07:07Z
dc.date.available 2011-01-14T10:07:07Z
dc.date.issued 2007
dc.identifier.isbn 978-86-80019-17-8 en_US
dc.identifier.uri http://hdl.handle.net/123456789/1491
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2011-01-14T10:07:07Z No. of bitstreams: 1 S07.pdf: 2121607 bytes, checksum: c8380cfb98dfc8aae098fa9d847f5511 (MD5) en
dc.description.provenance Made available in DSpace on 2011-01-14T10:07:07Z (GMT). No. of bitstreams: 1 S07.pdf: 2121607 bytes, checksum: c8380cfb98dfc8aae098fa9d847f5511 (MD5) Previous issue date: 2007 en
dc.language.iso en en_US
dc.publisher Nenad Milovanović & Milan S. Dimitrijević, Astronomical Observatory, Belgrade en_US
dc.title The shape of the Fe K alfa spectral line in the case of partly obscured accretion disk en_US
mf.document.pages 16 en_US
mf.contributor.editor-in-chief Dimitrijević, S. Milan

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