Astron. Astrophys. Suppl. Ser. 140, 247-260
Send offprint request: D.F. Roscoe
School of Mathematics, Sheffield University, Sheffield, S3 7RH, UK
Received June 7; accepted September 6, 1999
Subsequently, MFB (1996) published the unreduced optical rotation curves for approximately another 1100 southern sky spirals and, undoubtedly, more will follow from various sources. For this reason, and because of the importance of having large numbers of accurately folded rotation curves for dynamical studies, we have developed the automatic folding algorithm described herein.
An uncompiled Fortran program (using NAG routines) and data files are available via http://www.shef.ac.uk/~ap1dfr. Download the text file "ReadMe'' and follow instructions.
Key words: methods: numerical -- galaxies: kinematics and dynamics
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