Velocity curve analysis of the spectroscopic binary stars RZ Cas, CC Cas, HS Her, HD 93917, V921 Her and Y Cygni by the artificial neural networks

Details Velocity curve analysis of the spectroscopic binary stars RZ Cas, CC Cas, HS Her, HD 93917, V921 Her and Y Cygni by the artificial neural networks Velocity curve analysis of the spectroscopic binary stars RZ Cas, CC Cas, HS Her, HD 93917, V921 Her and Y Cygni by the artificial neural networks

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009an....330..836k&link_type=abstract

Astronomische Nachrichten, Vol.330, Issue 8, p.836-842

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Binaries: Eclipsing, Binaries: Spectroscopic, Stars: Individual (Rz Cas, Cc Cas, Hs Her, Hd 93917, V921 Her, Y Cygni)

Scientific paper

We use an Artificial Neural Network (ANN) to derive the orbital parameters of spectroscopic binary stars. Using measured radial velocity data of six double-lined spectroscopic binary systems RZ Cas, CC Cas, HS Her, HD 93917, V921 Her and Y Cygni, we find corresponding orbital and spectroscopic elements. Our numerical results are in good agreement with those obtained by others using more traditional methods.

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