| 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 |
|