First hot corino detected around an isolated intermediate-mass protostar: Cep E-mm

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Volume 618 (October 2018)

A&A, 618 (2018) A145

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Table 4.

Molecular species (COMs and chemically related species) detected with the IRAM 30 m telescope and the NOEMA interferometer.

Species	30m						NOEMA
	n	E_up (K)	Components			n	E_up (K)	Components
	n	E_up (K)	eBL	BL	NL	n	E_up (K)	eBL	BL
E-CH₃OH	72	4.6–500.5	×	×	×	4	37.6–500.5	×	×
A-CH₃OH	64	7.0–446.5	×	×	×	2	373.9–745.6		×
¹³CH₃OH	21	6.8–113.5		×		1	162.4		×
CH₂DOH	36	6.2–123.7		×	×	4	10.6–58.7	×	×
H₂CO	15	3.5–125.8	×	×	×	3	21.0–68.1	×	×
	9	10.2–61.3	×	×	×	1	32.9	×	×
H₂CCO	18	9.7–102.1		×	×	1	76.5	×	×
HCOOH	6	10.8–23.5			×	1	58.6		×
HCOOCH₃	24	20.1–111.5		×		16	20.1–111.5		×
CH₃CHO	63	7.6–89.8	×		×	1	18.3		×
CH₃OCH₃	30	11.1–106.3		×		1	253.4		×
CH₃COCH₃	0					1	119.1		×
HNCO	18	10.5–82.3	×		×	3	58.0–231.1	×	×
NH₂CHO^a	6	10.2–22.1			×	1	60.8		×
CH₃CN	38	8.8–148.6		×	×	^*
C₂H₅CN	0					2	135.6–139.9		×

Notes. For each species, we indicate the number n of detected transitions, the corresponding range of E_up and the detected spectral component with the 30 m: extremely broad line (eBL) component, the broad line (BL) component, and the narrow line (NL) component.

^(a)

30 m lines from López-Sepulcre et al. (2015).

^(∗)

No transition present in the band.

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