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- W157470740 abstract "Deep optical images of the circumstellar envelope of IRC+10216 have been obtained with CFHT and HST, with angular resolutions of 1 and 0.1, respectively. In the outer regions, the envelope is seen in dust-scattered galactic light, and is detected up to ∼200 from the star, corresponding to 8000 years of expansion. The envelope is composed of discrete, nearly circular, thin, limb-brightened shells. These shells are spaced at irregular intervals, and the shell/intershell density contrast is typically 3. Although the HST observations show a distinct bipolar geometry very near the star, the global shell pattern suggests a roughly isotropic, episodic mass loss mechanism." @default.
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- W157470740 date "2001-01-01" @default.
- W157470740 modified "2023-09-25" @default.
- W157470740 title "The Envelope of IRC+10216 Seen at High Angular Resolution" @default.
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- W157470740 doi "https://doi.org/10.1017/s0074180900221311" @default.
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