Synthetic brightness profiles resulting from consistent dynamical models for circumstellar dust shells around long-period variables are presented and discussed with respect to a corresponding observation of IRC + 10216.
机构:
INAF Ctr Galileo Galilei, Santa Cruz De La Palma 38700, TF, Spain
INAF Osservatorio Astron Catania, Catania, ItalyINAF Osservatorio Astron Padova, I-35122 Padua, Italy
Cosentino, R.
Scuderi, S.
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机构:
INAF Osservatorio Astron Catania, Catania, ItalyINAF Osservatorio Astron Padova, I-35122 Padua, Italy