SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 337, 517-538 (1998)

Previous Section Next Section Title Page Table of Contents

Acknowledgements

We acknowledge stimulating conversations with R. Bachiller, F. Bertoldi, P. Cox, T. Oliva, M. Perinotto, A. Tielens and M. Walmsley in the long course of preparing this paper. B. Draine kindly ran a version of his PDR code which had a more detailed calculation of H2 line intensities, in order to verify the accuracy of our various approximations for the individual H2 line intensities. Some of this work was done while AN was visiting the astronomy department of the University of California at Berkeley. DJH acknowledges travel support from ASI grants 92-RS-54, 94-RS-152 and 94-RS-152 to the Osservatorio di Arcetri and research support from the NASA Astrophysical Theory Program.

Previous Section Next Section Title Page Table of Contents

© European Southern Observatory (ESO) 1998

Online publication: August 17, 1998
helpdesk.link@springer.de