Evolution of complex organic molecules in hot molecular cores - Synthetic spectra at (sub-)mm wavebands

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Table 3

Abundance of COMs in Hot molecular cores: observed and simulated values.

Molecules	IRAS 16 293-2422¹	Orion Hot	NGC 6334I³	G29.96⁴	G327.3-0.6⁵	Garrod et al.	Garrod
		Core²				(2008)	(2013)

CH₃OH	3.0(–7)	2.2(–6)	4.7(–6)	6.6(–8)	5.3(–8)	3.2(–6)	1.1(–5)
C₂H₅OH	–	–	4.7(–8)	1.0(–8)	2.6(–9)	1.5(–9)	5.9(–8)
CH₃OCH₃	2.4(–7)	6.8(–8)	1.0(–6)	3.3(–8)	3.4(–7)	3.0(–9)	4.8(–8)
HCOOCH₃	2.0(–7)	–	2.4(–7)	1.3(–8)	5.0(–8)	7.8(–11)	9.2(–8)

Reference.

⁽¹⁾

Cazaux et al. (2003);

⁽²⁾

Crockett et al. (2014);

⁽³⁾

Zernickel et al. (2012);

⁽⁴⁾

Beuther et al. (2009);

⁽⁵⁾

Gibb et al. (2000a).

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