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Hα Observations of the Binary System VV Cephei Ernst Pollmann

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Presentation on theme: "Hα Observations of the Binary System VV Cephei Ernst Pollmann"— Presentation transcript:

1 Hα Observations of the Binary System VV Cephei Ernst Pollmann
ASPA Active Spectroscopy in Astronomy

2 VV Cephei 4,9 mag µ Cephei 4,0 mag
3 VV Cephei 4,9 mag µ Cephei 4,0 mag 1

3 1a

4 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

5 Rotating Hydrogen-Gasdisk and its hot Be-Star with 8 Solarmasses
blue shiftet red shiftet Observer 3

6 4

7 5

8 Time behavior of the Hα-emission since 1996 until today
Eclipse 6

9 V/R of the Hα-emission as function of orbital phase
7

10 Periastron passage 8 08/199401/2015 09/1999 09/2003 11/2009 10/2004
11/2005 8

11 Increase of the emission strength by mass overflow into the Be-disk at periastron
9

12 thanks for attention 14


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