Physical and chemical structure of high-mass star-forming regions - Unraveling chemical complexity with CORE: the NOEMA large program

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Volume 648 (April 2021)

A&A, 648 (2021) A66

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Table G.1

MUSCLE results for all three initial condition models.

	HMPO model			HMC model			UCHII model

Core	τ_chem	χ²	ϒ	τ_chem	χ²	ϒ	τ_chem	χ²	ϒ
	(yr)		(%)	(yr)		(%)	(yr)		(%)
IRAS 23033 1	33 574	0.339	64	73 271	0.346	64	97 675	0.336	64
IRAS 23033 2	18 019	0.525	64	49 046	0.589	64	104 065	0.589	55
IRAS 23033 3	18 705	0.517	64	50 019	0.559	64	96 415	0.567	64
IRAS 23151 1	19 415	0.458	64	49 222	0.557	64	83 510	0.444	82
IRAS 23385 1	17 547	0.581	55	48 510	0.498	55	87 011	0.644	45
IRAS 23385 2	20 729	0.545	55	48 510	0.602	45	95 268	0.465	55
AFGL 2591 1	17 884	0.508	64	54 635	0.562	64	83 510	0.441	82
CepA HW2 1	18 705	0.602	55	48 530	0.605	55	83 510	0.478	64
CepA HW2 2	19 415	0.459	73	48 812	0.616	45	88 141	0.454	73
G084.9505 1	16 510	0.475	55	48 510	0.533	55	83 510	0.537	55
G094.6028 1	17 884	0.593	55	56 611	0.521	64	83 784	0.536	55
G100.38 1	18 705	0.483	64	54 090	0.459	64	83 602	0.432	73
G108.75 1	20 011	0.485	73	48 602	0.608	55	87 011	0.610	55
G108.75 2	20 729	0.319	73	60 268	0.325	73	106 070	0.296	73
G075.78 1	18 330	0.471	64	49 547	0.532	64	84 222	0.410	82
IRAS 21078 1	17 157	0.602	73	55 234	0.509	64	92 402	0.516	73
IRAS 21078 2	18 168	0.601	55	48 876	0.542	64	84 884	0.575	55
NGC7538 IRS9 1	17 884	0.502	73	71 070	0.521	73	84 292	0.447	82
S87 IRS1 1	16 784	0.383	64	59 223	0.337	64	83 510	0.413	64
W3 H2O 3	17 547	0.590	55	48 876	0.579	45	83 510	0.532	64
W3 H2O 4	17 292	0.514	55	54 635	0.563	64	85 920	0.485	73
W3 IRS4 1	20 011	0.492	64	67 238	0.570	64	86 415	0.469	82

Notes. The best-fit chemical age τ_chem, χ² value, and percentage of well modeled molecules ϒ are shown for each initial condition model.

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