Complex molecule formation in grain mantles | Astronomy & Astrophysics (A&A)

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Table 1:

Observed fractional abundances of complex molecules.
Source - Hot Core	CH₃OH	C₂H₅OH	CH₃OCH₃
NGC6334F	$2.0\times10^{-7}$	$9.0\times10^{-9}$	$4.0\times10^{-8}$
NGC6334F	$1.0\times10^{-7}$	$1.0\times10^{-8}$	$3.0\times10^{-8}$
NGC6334F	$9.0\times10^{-8}$	$2.0\times10^{-8}$	$2.0\times10^{-8}$
NGC6334F	$9.0\times10^{-8}$	$6.0\times10^{-9}$	$1.0\times10^{-8}$
NGC6334F	$2.0\times10^{-7}$	$1.0\times10^{-8}$	$3.0\times10^{-8}$
NGC6334F	$2.0\times10^{-8}$	$1.0\times10^{-9}$	$7.0\times10^{-10}$
NGC6334F	$1.0\times10^{-8}$
NGC6334F	$4.0\times10^{-8}$
NGC6334F	$3.0\times10^{-7}$	$9.0\times10^{-9}$
NGC6334F	$2.0\times10^{-7}$
NGC6334F	$1.0\times10^{-6}$	$2.0\times10^{-8}$
Source - Hot Corino
NGC6334F	$1.0\times10^{-7}$		$2.4\times10^{-7}$
NGC6334F	< $1.0\times10^{-8}$		< $2.8\times10^{-8}$
NGC6334F	$7.0\times10^{-7}$		< $1.2\times10^{-6}$
NGC6334F	$3.0\times10^{-7}$		$3.0\times10^{-8}$

Notes. Data from Ikeda et al. (2001); Ikeda et al. (2002); Bottinelli et al. (2007).

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