During a very short period of clear sky, i started with the spectroscopic observations of Pleione (28 Tau) for a project in order to study the disk precession as a consequence of the periastron passages (BESS database et E.Pollmann)
During a very short period of clear sky, i started with the spectroscopic observations of Pleione (28 Tau) for a project in order to study the disk precession as a consequence of the periastron passages (BESS database et E.Pollmann)