CORRELATION BETWEEN X - RAY CONTINUUM AND Fe K (alfa) LINE VARIATION DUE TO MICROLENSING

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CORRELATION BETWEEN X - RAY CONTINUUM AND Fe K (alfa) LINE VARIATION DUE TO MICROLENSING

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dc.contributor.author Jovanović, P.
dc.contributor.author Popović, L. Č.
dc.contributor.author Dimitrijević, S. Milan
dc.contributor.editor Popović, L. Č.
dc.contributor.editor Milovanović, Nenad
dc.date.accessioned 2010-12-31T10:04:43Z
dc.date.available 2010-12-31T10:04:43Z
dc.date.issued 2003
dc.identifier.uri http://hdl.handle.net/123456789/1430
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2010-12-31T10:04:42Z No. of bitstreams: 1 26 Jovanovic, et al.pdf: 204083 bytes, checksum: fe35b06102879f71fc125a5e2fcf00ca (MD5) en
dc.description.provenance Made available in DSpace on 2010-12-31T10:04:43Z (GMT). No. of bitstreams: 1 26 Jovanovic, et al.pdf: 204083 bytes, checksum: fe35b06102879f71fc125a5e2fcf00ca (MD5) Previous issue date: 2003 en
dc.language.iso en en_US
dc.publisher Obs. Astron. Belgrade en_US
dc.title CORRELATION BETWEEN X - RAY CONTINUUM AND Fe K (alfa) LINE VARIATION DUE TO MICROLENSING en_US
mf.document.pages 6 en_US
mf.contributor.editor-in-chief Dimitrijević, S. Milan

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