A Possibility of Using Doppler Tomography to Indicate the Presence of Fluctuations and Structure Formations in Accretion Binary Systems (Conf. V)

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A Possibility of Using Doppler Tomography to Indicate the Presence of Fluctuations and Structure Formations in Accretion Binary Systems (Conf. V)

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dc.contributor.author Boneva, D.
dc.contributor.editor Tsvetkov, M. K.
dc.contributor.editor Filipov, L. G.
dc.contributor.editor Dimitrijević, M. S.
dc.contributor.editor Popović, L. Č.
dc.date.accessioned 2010-07-12T08:34:36Z
dc.date.available 2010-07-12T08:34:36Z
dc.date.issued 2007
dc.identifier.uri http://hdl.handle.net/123456789/831
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2010-07-12T08:34:36Z No. of bitstreams: 1 Boneva.pdf: 377202 bytes, checksum: 34da794e78d7f370652111213028e9d1 (MD5) en
dc.description.provenance Made available in DSpace on 2010-07-12T08:34:36Z (GMT). No. of bitstreams: 1 Boneva.pdf: 377202 bytes, checksum: 34da794e78d7f370652111213028e9d1 (MD5) Previous issue date: 2007 en
dc.language.iso en en_US
dc.publisher Heron Press Ltd, Sofia en_US
dc.title A Possibility of Using Doppler Tomography to Indicate the Presence of Fluctuations and Structure Formations in Accretion Binary Systems (Conf. V) en_US
mf.document.pages 7 en_US

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