The method of spectra disentangling and its links to Dopppler tomography.
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F01%3A01010155" target="_blank" >RIV/67985815:_____/01:01010155 - isvavai.cz</a>
Result on the web
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DOI - Digital Object Identifier
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Alternative languages
Result language
angličtina
Original language name
The method of spectra disentangling and its links to Dopppler tomography.
Original language description
The method of spectra disentangling fits time series of spectra of multiple stellar systems by a superposition of a priori unknown component spectra with Doppler shifts due to orbital motion with orbital parameters not known in advance. The method of Fourier disentangling, which solves simultaneously both parts of the problem, can also be used for Doppler tomography.
Czech name
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Czech description
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Classification
Type
C - Chapter in a specialist book
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/IAA3003805" target="_blank" >IAA3003805: Spectroscopic studies of binary and multiple starts</a><br>
Continuities
P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)
Others
Publication year
2001
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Book/collection name
Astrotomography. Indirect imaging methods in observational astronomy.
ISBN
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Number of pages of the result
8
Pages from-to
261-268
Number of pages of the book
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Publisher name
Springer
Place of publication
Berlin
UT code for WoS chapter
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