Class I and Class II methanol masers in high-mass star-forming regions

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Table B.5:

Same as Table B.4 for the 95 GHz CH₃OH maser (Class I) detected with the Nobeyama 45-m telescope.
Source^a	$V_{\rm LSR}$	$\int F_\nu {\rm d}V$	V	$\Delta V$	$F_{\nu}^{\rm peak}$
	(km s^-1)	(Jy km s^-1)	(km s^-1)	(km s^-1)	(Jy)
H05480+2545	-9.3^b	3.1 $\pm$ 0.6	-10.6 $\pm$ 0.1	1.3 $\pm$ 0.3	2.2
H18089-1732	32.9	2.7 $\pm$ 0.4	31.38 $\pm$ 0.02	0.45 $\pm$ 0.05	5.5
		14 $\pm$ 2	32.4 $\pm$ 0.2	3.2 $\pm$ 0.4	4.2
H18159-1648	22.1	4.7 $\pm$ 0.8	20.1 $\pm$ 0.1	1.6 $\pm$ 0.4	2.7
		7.6 $\pm$ 0.6	22.56 $\pm$ 0.06	1.4 $\pm$ 0.1	5.2
H18316-0602	42.2	1.1 $\pm$ 0.2	41.63 $\pm$ 0.05	0.5 $\pm$ 0.1	2.1
H18360-0537	102.3	13.2 $\pm$ 0.8	102.5 $\pm$ 0.1	4.1 $\pm$ 0.4	4.0
H20126+4104	-3.9	6.0 $\pm$ 0.4	-2.75 $\pm$ 0.08	2.3 $\pm$ 0.2	2.5
H21391+5802	0.4	2.5 $\pm$ 0.6	12.1 $\pm$ 0.1	1.2 $\pm$ 0.5	2.0
H22506+5944	-51.5	5 $\pm$ 1	-47.1 $\pm$ 0.2	2.4 $\pm$ 0.6	2.0
L18018-2426	10.5	33.5 $\pm$ 0.4	10.800 $\pm$ 0.004	0.622 $\pm$ 0.009	50
L18144-1723	47.3	26.4 $\pm$ 0.6	47.91 $\pm$ 0.03	2.07 $\pm$ 0.08	12
L18396-0431	97.3	3.8 $\pm$ 0.4	50.37 $\pm$ 0.08	1.24 $\pm$ 0.2	2.9
		14 $\pm$ 2	57.4 $\pm$ 0.6	7 $\pm$ 1	1.9
		4 $\pm$ 1	61.5 $\pm$ 0.1	1.3 $\pm$ 0.4	2.5
		8.0 $\pm$ 0.8	71.3 $\pm$ 0.2	3.4 $\pm$ 0.6	2.2
		1.6 $\pm$ 0.2	130.50 $\pm$ 0.08	0.7 $\pm$ 0.1	2.1

Notes. ^(a) ``L'' and ``H'' indicate if the source belongs to the low or high sample; ^(b) from NH₃ observations performed with the Nobeyama 45-m telescope.

Source LaTeX | All tables | In the text

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