We report H-alpha observations of zeta Tauri, taken between late 2000 and early 2006. Next to extending existing long-term montioring of the disk state of this star we report an intermediate timescale of about 69 days to be present in the V/R variations of the Halpha line. The observational data will be published together with this manuscript.
Cite
@article{arxiv.0801.4530,
title = {H-alpha observations of zeta Tauri},
author = {E. Pollmann and Th. Rivinius},
journal= {arXiv preprint arXiv:0801.4530},
year = {2008}
}
Comments
7 pages, 5 figures, accepted by the IBVS as No. 5813