Molecular outflows and hot molecular cores in G24.78+0.08 at sub-arcsecond angular resolution

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Table 1

Parameters of the maps.

			Synthesized beam^a

		Frequency	HPBW	PA	Spectral resolution	rms noise^b
Observation	Telescope^a	(GHz)	(arcsec)	(deg)	(km s^-1)	(mJy beam^-1)

continuum	SMA	225.31	0.95 × 0.75^c	61^c	–	3.0^c
continuum	PdBI	214.30	0.89 × 0.29	10	–	3.2
¹³CH₃CN (12_K–11_K)	PdBI	214.374^d	0.89 × 0.29^e	10	0.25	15
C¹⁸O (2–1)	SMA	219.560	0.83 × 0.64^e	55	0.6	35
HNCO (10_0,10–9_0,9)	SMA	219.798	0.72 × 0.51	46	0.6	45
H₂¹³CO (3_1,2–2_1,1)	SMA	219.909	0.72 × 0.51	46	0.6	45
SO (6₅–5₄)	SMA	219.949	0.83 × 0.64^e	55	0.6	40
CH₃OH (8_0,8–7_1,6)	SMA	220.079	0.66 × 0.48	48	0.6	45
HCOOCH₃ (17_2,15–16_4,2)	SMA	220.167	0.71 × 0.50	45	0.6	45
CH₂CO (1_1,11–10_1,10)	SMA	220.178	0.71 × 0.50	45	0.6	45
HCOOCH₃ (17_4,13–16_4,12)	SMA	220.190	0.71 × 0.50	45	0.6	45
¹³CO (2–1)	SMA	220.399	0.83 × 0.64^e	55	1.0	35
¹³CO (2–1)	SMA+IRAM 30-m	220.399	3.57 × 2.02	71	1.0	116
CHCN (12_K–11_K)	SMA	220.638^d	0.67 × 0.47	47	0.6	45
C₂H₅CN (25_2,24–24_2,23)	SMA	220.661	0.67 × 0.48	47	0.6	45
CH₃CN (12_K–11_K)	SMA	220.747^d	0.71 × 0.50	46	0.6	40
CH₃CN v₈ = 1 ( K,l = 6, + 1)	SMA	221.312	0.66 × 0.47	46	0.6	40
CH₃CN v₈ = 1 (K,l = 3, − 1)	SMA	221.338	0.66 × 0.47	46	0.6	40
CH₃OH (8_1,8–7_0,7)E	SMA	229.759	0.65 × 0.47	48	0.6	50
CH₃OH (19_5,14–20_4,17)A −	SMA	229.939	0.65 × 0.47	47	0.6	45
CH₃OH (3_2,2–4_1,4)E	SMA	230.027	0.65 × 0.47	48	0.6	45
¹²CO (2–1)	SMA	230.538	0.86 × 0.68^e	54	1.5	40
¹²CO (2–1)	SMA+IRAM 30-m	230.538	3.37 × 1.96	70	1.0	116
OCS (19–18)	SMA	231.061	0.69 × 0.50	46	0.6	50
¹³CS (5–4)	SMA	231.221	0.70 × 0.49	46	0.6	50

Notes.

^(a)

The synthesized CLEANed beams for maps with the ROBUST parameter of Briggs (1995) set equal to 0;

^(b)

for the molecular line observations the 1σ noise is per channel;

^(c)

the synthesized beam for the SMA VEX configuration map is at PA = 52°, and the rms noise is 3.2 mJy beam^-1;

^(d)

the frequency is that of the K = 0 component;

^(e)

the synthesized CLEANed beams for maps using natural weighting.

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