0124902 - ASU-R 20010155 RIV DE eng M - Část monografie knihy
Hadrava, Petr
The method of spectra disentangling and its links to Dopppler tomography.
Astrotomography. Indirect imaging methods in observational astronomy. Berlin: Springer, 2001 - (Boffin, H.; Steeghs, D.; Cuypers, J.), s. 261-268. Lecture notes in physics., 573
Grant CEP: GA AV ČR IAA3003805
Výzkumný záměr: CEZ:AV0Z1003909
Klíčová slova: spectra disentangling * stellar systems * Doppler tomography
Kód oboru RIV: BN - Astronomie a nebeská mechanika, astrofyzika

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.
Trvalý link: http://hdl.handle.net/11104/0023161