A&A Supplement series, Vol. 122, April II 1997, 285-292
Received October 4, 1995; accepted July 30, 1996
M. Lemke
Send offprint request: M. Lemke, Bamberg address
Institute of Astronomy, Madingley Road, Cambridge CB3 0HA,
UK
e-mail: michael@astro.as.utexas.edu
We announce the availability of Stark broadening tables for the
Lyman, Balmer, Paschen, and Brackett series of hydrogen, computed with
the VCS theory (Vidal et al. 1973). The tables cover the
series up to n=22 and an extended grid of 
and T, with T
running as high as 160000K, suitable for central stars of Planetary
Nebulae and similar.
keywords: atomic data -- line: profiles