NEWS
Campaign Periastron Passages of Pleione
VV Cep up-to-date: 2019-09-20
The current state of the ARAS campaign observation results seems to explain the periodic time behavior of the equivalent width EW and the flux of the Hα emission components V&R.
Based on these results, a new geometric structure of the emission sources has been developed in collaboration with Prof. Dr. Ph. Bennett (Dalhousie University, Halifax, NS, Canada).
Link to the animation: disk axis precession
P Cygni up-to-date
Photometry and Spectroscopy of P Cygni: Periodic Variation of the intrinsic Halpha-line flux
New Publications
1) The Long-term Binary System VV Cep
2) Monitoring the radial velocity of He 6678 of gamma Cas
3) Radial velocity of the HeI 6678 Line of zeta Tau
4) A Time Series of BV Photometry and Halpha Emission Fluxes of the Eclipsing Binary VV Cep
5) Correlation of Halpha Emission Flux with B & V Magnitudes for VV Cep
6) Mass & precession of the disk in zeta Tau
7) Evolution of the disk of pi Aqr: From near disappearance to a strong maximum
8) Photometry and Spectroscopy of P Cygni: Periodic Variation of the intrinsic Halpha-line flux