We present visual and CCD VRI observations of a suspected symbiotic binary V335 Vul. Long term photometry suggests usual Mira or SRa pulsations. High speed V band CCD photometry didn't reveal anything unusual above 0.02 mag.
@article{arxiv.astro-ph/0210585,
title = {Observations of possible symbiotic star V335 Vul},
author = {Petr Sobotka and Ondrej Pejcha and Ladislav Smelcer and Pavel Marek},
journal= {arXiv preprint arXiv:astro-ph/0210585},
year = {2007}
}
Comments
4 pages, 2 Postscript figures, to appear in the proceedings of "Symbiotic stars probing stellar evolution", R.L.M.Corradi, J.Mikolajewska, T.J.Mahoney eds., 2002, ASP Conference Series, in press