The hot corino-like chemistry of four FUor-like protostars

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Table 2

Positions of the protostars and the pixels used to extract the spectra, and the separation between the two positions.

Target	Protostar coordinates	Spectra coordinates	Separation (″)	v_sys (km s⁻¹)
L1551 IRS 5 N	04:31:34.1623 +18:08:04.717	04:31:34.1575 +18:08:04.793	0.102	7.56
L1551 IRS 5 S	04:31:34.1664 +18:08:04.356	04:31:34.1669 +18:08:04.253	0.103	5.16
Haro 5a IRS	05:35:26.5594 −05:03:55.130	05:35:26.5616 −05:03:55.064	0.074	14.06
V346 Nor	16:32:32.1971 −44:55:30.769	16:32:32.1951 −44:55:30.769	0.021	−4.58
OO Ser	18:29:49.1515 +01:16:19.676	18:29:49.1535 +01:16:19.646	0.042	8.22

Notes. The v_LSR at the coordinates where we extracted the spectra is measured on the bright H₂S 2(2,0)–2(1,1) transition at 216.71 GHz detected in these observations.

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