Reconstruction of the Structure of Cataclysmic Variables from Observations

Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F19%3A10407013" target="_blank" >RIV/00216208:11320/19:10407013 - isvavai.cz</a>
Výsledek na webu
<a href="https://www.mff.cuni.cz/veda/konference/wds/proc/pdf19/WDS19_27_f1_Kara.pdf" target="_blank" >https://www.mff.cuni.cz/veda/konference/wds/proc/pdf19/WDS19_27_f1_Kara.pdf</a>
DOI - Digital Object Identifier
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Jazyk výsledku
angličtina
Název v původním jazyce
Reconstruction of the Structure of Cataclysmic Variables from Observations
Popis výsledku v původním jazyce
We present an overview of methods for the study of the structure of cataclysmic variables. One method is based on the analysis of photometric observation of eclipses of studied objects. By light-curve modelling, properties of the system can be determined. Another method, the Doppler tomography, is based on analysis of time-resolved spectra and can provide an insight into to the properties of the emission region of the accretion disc of a cataclysmic variable. We show the study of a dwarf nova CzeV404 Her as an example for these methods.
Název v anglickém jazyce
Reconstruction of the Structure of Cataclysmic Variables from Observations
Popis výsledku anglicky
We present an overview of methods for the study of the structure of cataclysmic variables. One method is based on the analysis of photometric observation of eclipses of studied objects. By light-curve modelling, properties of the system can be determined. Another method, the Doppler tomography, is based on analysis of time-resolved spectra and can provide an insight into to the properties of the emission region of the accretion disc of a cataclysmic variable. We show the study of a dwarf nova CzeV404 Her as an example for these methods.

Rok uplatnění
2019
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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