Spectroscopy and doppler mapping of the binary SS Cyg during outburst

We carried out spectroscopy of the binary SSCyg in the H α , H β , and H γ lines in its active state in August and December 2006. We have estimated the parameters of the main flow elements contributing to the spectra. Profile variations during the orbital period are analyzed, and a Doppler tomogram...

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Veröffentlicht in:	Astronomy reports 2008-10, Vol.52 (10), p.835-846
Hauptverfasser:	Kononov, D. A., Kaigorodov, P. V., Bisikalo, D. V., Boyarchuk, A. A., Agafonov, M. I., Sharova, O. I., Sytov, A. Yu, Boneva, D.
Format:	Artikel
Sprache:	eng
Schlagworte:	Accretion Astronomy Astrophysics Double stars Observations and Techniques Orbits Phenomenology Physics Physics and Astronomy Spectroscopy Spectrum analysis
Online-Zugang:	Volltext
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