On the Stark Broadening of Visible Ar I Lines for Astrophysical Plasma Analysis and Modelling

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On the Stark Broadening of Visible Ar I Lines for Astrophysical Plasma Analysis and Modelling

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dc.contributor.author Christova, M.
dc.contributor.author Dimitrijević, M.
dc.contributor.author Sahal-Brechot, S.
dc.contributor.author Andreev, N.
dc.date.accessioned 2013-12-02T10:09:07Z
dc.date.available 2013-12-02T10:09:07Z
dc.date.issued 2007
dc.identifier.uri http://hdl.handle.net/123456789/3280
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2013-12-02T10:09:07Z No. of bitstreams: 1 5BGSCASD_187_2007_Christova.pdf: 167802 bytes, checksum: 9bc3bd0e811948a09cdde217f3b935dc (MD5) en
dc.description.provenance Made available in DSpace on 2013-12-02T10:09:07Z (GMT). No. of bitstreams: 1 5BGSCASD_187_2007_Christova.pdf: 167802 bytes, checksum: 9bc3bd0e811948a09cdde217f3b935dc (MD5) Previous issue date: 2007 en
dc.language.iso en en_US
dc.publisher Sofia en_US
dc.title On the Stark Broadening of Visible Ar I Lines for Astrophysical Plasma Analysis and Modelling en_US
mf.document.pages 5 en_US

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