A comparative study of high-mass cluster forming clumps

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Volume 517 (July 2010)

A&A, 517 (2010) A66

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Table A.2:

Gaussian fit to C¹⁸O(2-1) spectra at peak coordinates $^{\ast }$ .
Source	$V_{{\rm LSR}}$	$\it FWHM$	$T_{\rm MB}$	$\int T_{\rm MB} {\rm d}V$
	(km s^-1)	(km s^-1)	(K)	(K km s^-1)
05358+3543	-16.7 (0.2)	4.2 (0.5)	2.9 (0.5)	13.0 (1.3)
G213.61-12.6	10.0 (0.1)	2.7 (0.2)	7.6 (0.6)	21.6 (1.1)
G189.78+0.34	9.0 (0.1)	3.0 (0.1)	6.9 (0.4)	22.1 (0.9)
G192.58-0.04	9.1 (0.1)	2.9 (0.3)	8.8 (0.7)	27.0 (0.5)
G192.60-0.05	7.4 (0.1)	3.3 (0.2)	7.4 (0.6)	25.9 (1.1)
18151-1208_2^b	30.0 (0.4)	3.5 (1.0)	3.3 (1.3)	12.5 (2.8)
18151-1208_3	30.4 (0.1)	1.4 (0.1)	10.5 (0.2)	15.1 (1.2)
18151-1208_1	33.6 (0.2)	3.3 (0.4)	9.8 (1.5)	34.4 (3.4)
G18.15-0.28	55.2 (0.1)	3.2 (0.1)	13.4 (0.7)	46.3 (1.3)
G18.18-0.30	50.1 (0.1)	3.0 (0.2)	10.0 (0.9)	31.7 (1.6)
18223-1243	45.0 (0.1)	3.0 (0.1)	13.0 (0.9)	40.8 (1.7)
18228-1312	33.1 (0.1)	4.2 (0.2)	8.5 (0.6)	37.5 (1.4)
G19.27+0.1M2	26.8 (0.1)	2.3 (0.3)	3.7 (0.6)	9.1 (0.9)
G19.27+0.1M1^a	26.3 (0.2)	1.7 (0.3)	2.8 (0.8)	5.2 (1.1)
18236-1205	26.3 (0.1)	3.3 (0.1)	9.2 (0.5)	32.6 (1.0)
18264-1152	43.8 (0.1)	3.1 (0.4)	7.7 (1.1)	25.8 (2.5)
G23.60+0.0M1	106.0 (0.1)	3.7 (0.3)	6.6 (0.5)	25.5 (1.5)
18316-0602	42.6 (0.1)	4.8 (0.2)	8.0 (0.6)	41.3 (1.5)
G23.60+0.0M2	53.5 (0.1)	2.9 (0.3)	4.3 (0.6)	13.2 (1.1)
18317-0513	41.7 (0.1)	2.3 (0.1)	9.9 (0.6)	24.8 (1.0)
G24.08+0.0M2	51.9 (0.3)	1.9 (0.5)	3.2 (1.2)	6.4 (1.7)
G24.33+0.1M1	112.9 (0.1)	3.5 (0.3)	5.1 (0.7)	19.1 (1.4)
G24.33+0.1M4^c	114.0 (0.3)	5.5 (0.7)	2.6 (0.3)	15.3 (1.8)
G24.33+0.1M2	117.7 (0.2)	3.8 (0.4)	3.3 (0.6)	13.2 (1.2)
G24.60+0.1M2^c	114.6 (0.2)	3.7 (0.6)	4.1 (0.5)	16.1 (2.2)
G24.60+0.1M1	53.6 (0.1)	2.8 (0.3)	3.6 (0.4)	10.6 (1.0)
G25.04-0.2M1	63.6 (0.1)	2.2 (0.2)	6.3 (0.4)	14.8 (0.9)
G25.04-0.2M4^a,b	62.9 (0.4)	2.5 (1.0)	2.7 (1.5)	7.1 (2.5)
G25.04-0.2M2	63.3 (0.1)	2.5 (0.3)	2.9 (0.4)	7.7 (0.8)
G28.28-0.35	48.2 (0.1)	3.6 (0.1)	7.6 (0.5)	29.0 (1.0)
18507+0121	58.0 (0.2)	6.0 (0.5)	6.9 (1.4)	43.4 (3.4)
G34.43+0.2M1	58.0 (0.3)	4.8 (0.8)	4.5 (1.2)	23.3 (2.8)
G34.43+0.2M3	58.5 (0.2)	2.3 (0.6)	4.1 (0.5)	10.1 (2.1)
G34.24+0.13	56.9 (0.1)	2.6 (0.1)	14.0 (0.5)	38.4 (0.8)
18517+0437	44.1 (0.1)	2.7 (0.3)	10.4 (1.6)	29.4 (2.7)
G34.77-0.6M2^b,d	43.2 (0.7)	6.2 (1.4)	1.0 (0.5)	6.4 (1.3)
G35.39-0.3M4^b	45.1 (0.2)	1.3 (0.3)	1.6 (0.2)	2.2 (0.6)
G38.95-0.5M1	42.2 (0.1)	3.1 (0.2)	5.7 (0.4)	19.0 (0.8)
19035+0641	32.8 (0.2)	5.7 (0.5)	3.0 (0.4)	18.0 (1.1)
19095+0930	43.9 (0.1)	5.8 (0.2)	8.8 (0.5)	54.7 (1.4)
20216+4107	-1.4 (0.1)	1.5 (0.2)	7.0 (0.5)	11.2 (1.0)
20332+4124	-2.6 (0.1)	3.0 (0.3)	6.9 (0.8)	21.9 (1.6)
22134+5834	-18.3 (0.1)	2.3 (0.1)	7.2 (0.6)	17.3 (0.9)
22570+5912_2^a,b	-48.5 (0.7)	3.2 (1.7)	1.9 (0.8)	6.4 (2.1)
22570+5912_1	-45.7 (0.1)	2.5 (0.3)	4.7 (0.6)	12.6 (1.0)
23033+5951	-53.6 (0.1)	3.1 (0.2)	6.4 (0.7)	20.9 (1.4)
23139+5939	-44.1 (0.1)	3.7 (0.2)	4.7 (0.5)	18.8 (1.0)
23151+5912	-54.6 (0.1)	3.2 (0.3)	5.5 (0.6)	18.6 (1.2)

Notes. $^{(\ast)}$ The errors are indicated in brackets; ^(a) fit to spectrum at HCO⁺(1-0) peak coordinates; (b) weak line and/or noisy spectrum: bad fit; (c) C¹⁸O line outside VESPA unit limits: 1 MHz spectrum used; (d) fit to spectrum at offset coordinates (-13.3'', -9.0'') (see HCO⁺(1-0) and HCN(1-0) integrated maps in Fig. B.1).

Source LaTeX | All tables | In the text

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