Table 1: Parameters of the OVRO observations.
Synthesized beam

Observation Configuration Frequency HPBW PA Bandwidth Spectral resolution rms noise^a

(GHz) (arcsec) (deg) (MHz) (km s^-1) (mJy beam^-1)

2.7 mm continuum L, C 112.53 $6.3\times4.8$ -27 4000 - 1.4

CO ( $J=1\rightarrow 0$ ) L, C 115.27 $8.0\times6.3$ -29 22.5 0.65 45

C¹⁸O ( $J=1\rightarrow 0$ ) L, C 109.78 $8.0\times6.6$ -32 7.5 0.68 40

HC₃N ( $J=12\rightarrow 11$ ) L, C 109.17 $8.1\times6.7$ -37 7.5 0.69 40

**Table 1:** Parameters of the OVRO observations.
			Synthesized beam
Observation	Configuration	Frequency	HPBW	PA	Bandwidth	Spectral resolution	rms noise^a
		(GHz)	(arcsec)	(deg)	(MHz)	(km s^-1)	(mJy beam^-1)
2.7 mm continuum	L, C	112.53	$6.3\times4.8$	-27	4000	-	1.4
CO ( $J=1\rightarrow 0$ )	L, C	115.27	$8.0\times6.3$	-29	22.5	0.65	45
C¹⁸O ( $J=1\rightarrow 0$ )	L, C	109.78	$8.0\times6.6$	-32	7.5	0.68	40
HC₃N ( $J=12\rightarrow 11$ )	L, C	109.17	$8.1\times6.7$	-37	7.5	0.69	40

^a For the molecular line observations the 1 $\sigma$ noise is per channel.

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