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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

  • DOI - Digital Object Identifier

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

  • Czech description

Classification

  • Type

    C - Chapter in a specialist book

  • CEP classification

    BN - Astronomy and celestial mechanics, astrophysics

  • OECD FORD branch

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

  • Number of pages of the result

    8

  • Pages from-to

    261-268

  • Number of pages of the book

  • Publisher name

    Springer

  • Place of publication

    Berlin

  • UT code for WoS chapter