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==> In this proposal, more time is being requested for JKOORNNE.ARACLUS
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We propose to investigate a unique galactic B[e] star in a heavily
reddened cluster in the ARA constellation. We have discovered with ISO
SWS very high excitation gas at a position near the B[e] star, and we also
discovered extended 10 micron emission with ISOCAM near another star in
the cluster, an M supergiant separated by about 14 arcsec from the B[e]
star. Recent radio observations show strong non-thermal radio emission
from the B[e] star and also from the M supergiant. We wish to
investigate the nature of the emission using ISOCAM and ISO-SWS.