Astron. Astrophys. 329, L53-L56 (1998)

Acknowledgements

The ISOPHOT data presented in this paper was reduced using PIA, which is a joint development by the ESA Astrophysics Division and the ISOPHOT consortium led by the Max Planck Institute for Astronomy (MPIA), Heidelberg. Do Kester provided valuable help in examining various IRAS data of  Cnc. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. CD acknowledges support from the Stichting Astronomisch Onderzoek (ASTRON, project nr. 781-76-015).

© European Southern Observatory (ESO) 1998

Online publication: December 16, 1997
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