Studying star-forming processes at core and clump scales: the case of the young stellar object G29.862−0.0044

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This article has an erratum: [https://doi.org/10.1051/0004-6361/202038243e]

Table 3

Tabulated and Gaussian fitting parameters (see Fig. 8) for the K projections of the CH₃CN J = 13–12 transition.

K	Frequency	E_u	S_ul μ²	I_peak	W
	(GHz)	(K)	(Debye²)	(Jy beam⁻¹)	(Jy beam⁻¹ km s⁻¹)
0	239.137	80.3	199.1	0.10	0.75
1	239.133	87.5	197.9	0.08	0.63
2	239.119	108.9	194.3	0.07	0.59
3	239.096	144.6	188.5	0.07	0.62

Notes. The central frequency takes into consideration the collapsed hyperfine components for each projection (spacing smaller than channel width).

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