Astron. Astrophys. 338, 340-352 (1998)

Acknowledgements

We thank Claes-Ingvar Lagerkvist, Per Magnusson and Anders Erickson for their comments and support in discussions about the HG-parameters, shape and spin vector solutions. We thank also the members of the ISOPHOT Instrument Dedicated Team in Villafranca and the ISOPHOT Data Centre in Heidelberg, especially D. Lemke, U. Klaas, B. Schulz and S. Huth, for the helpful discussions about the ISOPHOT data reduction, many useful comments and the explanation of the FCS tables.

We retrieved the submillimetre data from the JCMT archive at the Canadian Astronomy Data Centre, which is operated by the Dominion Astrophysical Observatory for the National Research Council of Canada's Herzberg Institute of Astrophysics. We thank D. Hughes and J. Stevens for sharing their experience with the submillimetre instrumentation and the data reduction.

The UKIRT observations have been performed by the MPIA MAX instrument team, namely S. V. W. Beckwith, M. Robberto, T. Herbst and P. Bizenberger.

We also would like to express our thanks to the referee, Dr. M. Cohen. His comments were very helpful and improved the paper significantly.

© European Southern Observatory (ESO) 1998

Online publication: September 8, 1998
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