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Neutral Carbon in the Protoplanetary Nebulae CRL 618 and CRL 2688
Author(s) -
Ken Young
Publication year - 1997
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/310926
Subject(s) - asymptotic giant branch , astrophysics , physics , carbon fibers , line (geometry) , astronomy , stars , materials science , geometry , mathematics , composite number , composite material
The 609u 3P1 -> 3P0 line of neutral atomic carbon has been detected in theprotoplanetary nebulae CRL 618 and CRL 2688. CI appears to be about 7% asabundant as CO in CRL 2688, and 70% as abundant as CO in CRL 618. CI emissionarises primarily from the slow component of the wind from these objects. Thedata presented here indicate that CI gradually becomes more abundant as thestar leaves the AGB, and CI is significantly enhanced relative to CO before thestar develops a large HII region.Comment: 7 pages, LaTex AASTeX macros. To appear in ApJ Letter

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