Publication Date:
2019-06-27
Description:
High-sensitivity emission profiles were observed for the transition of C12O16 and C13O16 towards IRC + or - 10216. It appears that the spherically symmetric uniform mass-outflow model proposed by Morris is necessary to describe the line profiles. The outflow appears to be slightly accelerated, having a velocity of 15 km/sec at the edges of the CO cloud, compared with 12 km/sec for the more centrally confined molecules.
Keywords:
ASTRONOMY
Type:
NASA-CR-119157
,
AD-A011098
,
REPT-1975-8
Format:
application/pdf
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