AN INFRARED STUDY OF THE REMARKABLE DUSTY M-STAR HR-3126

HR 3126 is a unique M giant star embedded in the bipolar reflection nebula IC 2220. Its evolutionary status is uncertain, and both the composition of the dust shell and the mechanism responsible for its ejection have proved controversial. In this paper we present new photometric and spectroscopic ob...

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Bibliografiska uppgifter
Huvudupphovsmän: Chiar, J, Whittet, D, Aitken, D, Roche, P, Smith, C, Walker, H, Whitelock, P, Wright, C
Materialtyp: Journal article
Språk:English
Publicerad: Institute of Physics Publishing 1993

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