Applications of Fourier disentangling on the spectra of multiple stars

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Applications of Fourier disentangling on the spectra of multiple stars

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dc.contributor.author Elner, Jan
dc.contributor.editor Kovačević, Andjelka
dc.date.accessioned 2011-01-25T10:04:01Z
dc.date.available 2011-01-25T10:04:01Z
dc.date.issued 2008
dc.identifier.isbn 978-86-80019-30-7 en_US
dc.identifier.uri http://hdl.handle.net/123456789/1555
dc.description.provenance Submitted by Slavisha Milisavljevic (slavisha) on 2011-01-25T10:04:01Z No. of bitstreams: 1 Elner.pdf: 739485 bytes, checksum: a9d1e6004fcc777c45bee051e501e9de (MD5) en
dc.description.provenance Made available in DSpace on 2011-01-25T10:04:01Z (GMT). No. of bitstreams: 1 Elner.pdf: 739485 bytes, checksum: a9d1e6004fcc777c45bee051e501e9de (MD5) Previous issue date: 2008 en
dc.language.iso en en_US
dc.publisher Astronomical Observatory Belgrade en_US
dc.title Applications of Fourier disentangling on the spectra of multiple stars en_US
mf.subject.keywords Fourier disentangling is one of progressive methods developed for decomposition of composite spectra of multiple stellar systems. We apply code KOREL (Hadrava, 2004) to study several stellar systems, to obtain individual spectra of their components, to precise their orbital parameters and even unreveal so far undetected components as well as suggest their physical nature. Secular changes of the orbital parameters can be studied as well. These calculations can be treated as a test of applicability, functionality and limitations of the presented method and some conclusions can be discussed. en_US
mf.document.pages 16 en_US
mf.contributor.editor-in-chief Dimitrijević, S. Milan
mf.contributor.technical-editor Milovanov, Tatjana

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