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Paper detail

New infrared object in the field of the SMC cluster NGC 330

We report ISO (Infrared Space Observatory) observations of a new infrared source discovered in the vicinity of the young populous cluster NGC 330 in the Small Magellanic Cloud. The object was observed with ISOCAM at 4.5, 6.75 and 11.5 $μ$m and shows a prominent mid-infrared excess, indicating the presence of a dust shell. The available observations of the optical counterpart together with the mid-infrared ISOCAM data suggest that this object is most likely a post-AGB star, or a Be supergiant. Cluster membership and candidate evolutionary scenarios are discussed briefly.

preprint1999arXivOpen access
A. KucinskasV. VanseviciusM. SauvageT. Tanabé
astro-ph
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Open access4 authors1 topic
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A. KucinskasV. VanseviciusM. SauvageT. Tanabé

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