Physics
Scientific paper
Apr 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8426518b&link_type=abstract
Unknown
Physics
Carbon, Carbon Stars, Nebulae, Neutral Atoms, Stellar Evolution, Stellar Spectrophotometry, Interstellar Matter, Radio Spectra, Stellar Envelopes, Stellar Mass Ejection
Scientific paper
A search for sub-mm C I emission from seven stars that are surrounded by dense molecular gas shells led to the detection, in the case of the "Egg Nebula' (AFGL 2688), of an 0.9 K line implying a C I/CO value greater than 5. The material surrounding this star must be extremely carbon-rich, and it is suggested that the apparently greater extent of the C I emission region may be due to the effects of the galactic UV field on the shell's chemistry, as suggested by Huggins and Glassgold (1982).
Alwyn Wootten H.
Beichman Charles Arnold
Frerking Margaret A.
Huggins Patrick J.
Keene Jocelyn
No associations
LandOfFree
Neutral carbon in the EGG Nebula (AFGL 2688) does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Neutral carbon in the EGG Nebula (AFGL 2688), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Neutral carbon in the EGG Nebula (AFGL 2688) will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1236472