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Dust around AFGL 2688, molecular shielding, and the production of carbon chain molecules

Journal Article · · Astrophysical Journal; (USA)
DOI:https://doi.org/10.1086/168457· OSTI ID:6851834
;  [1]
  1. California Univ., Los Angeles (USA)

The molecular, IR, and optical maps of the evolved carbon star AFGL 2688 (the Egg Nebula) are all consistent with a model of a bipolar outflow of approximately 0.0001 solar masses/yr that stopped as this object evolved beyond the asymptotic giant branch about 200 years ago. In order to explain the extended HC7N emission around this star, it is proposed that carbon grains are collisionally fragmented as they supersonically steam through the circumstellar envelope. 60 refs.

OSTI ID:
6851834
Journal Information:
Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 351; ISSN ASJOA; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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