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Hα Observations of the Binary System VV Cephei Ernst Pollmann
ASPA Active Spectroscopy in Astronomy
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VV Cephei 4,9 mag µ Cephei 4,0 mag
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M2Iab Supergiant 2-3 Solar masses 1600 Solar radii
The orbit of the Be-star + Gasdisk leads to the eclipse by the M-type star Duration of eclipse: 673 days Periode: 20,4 years M2Iab Supergiant Solar masses 1600 Solar radii Last eclipse: Jun/1996 – August/1998 2
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Rotating Hydrogen-Gasdisk and its hot Be-Star with 8 Solarmasses
blue shiftet red shiftet Observer 3
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Time behavior of the Hα-emission since 1996 until today
Eclipse 6
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V/R of the Hα-emission as function of orbital phase
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Periastron passage 8 08/199401/2015 09/1999 09/2003 11/2009 10/2004
11/2005 8
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Increase of the emission strength by mass overflow into the Be-disk at periastron
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thanks for attention 14
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