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Astron. Astrophys. 327, 1054-1069 (1997)

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Acknowledgements

The authors are very grateful to A. Cool, I. King, F. Paresce, G. DeMarchi, R. Elson and G. Gilmore, for kindly providing their data under electronic forms. We are particularly indebted to A. Cool, G. DeMarchi, F. Paresce, and J. Holtzman for sending us the WFPC2 555, 814 and 606 transmission filters and additional transformations, and to F. Rogers for computing opacities with [FORMULA] -enriched abundances upon request. We also thank C. Dahn for sending his tabulated data.

This work is funded by grants from NSF AST-9217946 to Indiana University and NASA LTSA NAG5-3435 and NASA EPSCoR NAG-3435 to Wichita State University. PHH was partially supported by NASA LTSA and ATP grants to the University of Georgia in Athens. The calculations presented in this paper were performed at the Cornell Theory Center (CTC), the San Diego Supercomputer Center (SDSC), and on the CRAY C90 of the Centre d'Etudes Nucléaire de Grenoble.

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© European Southern Observatory (ESO) 1997

Online publication: April 6, 1998
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