VLBI study of maser kinematics in high-mass star-forming regions - II. G23.01–0.41

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Table 1:

G23.01-0.41: radio continuum emission.
					Peak position^a
Telescope	$\lambda$	HPBW	PA	Image rms	RA(J2000)	Dec(J2000)	$F_{\rm peak}$	$F_{\rm int}$
	(cm)	( $'' \times ''$ )	( $^\circ$ )	(mJy beam^-1)	(h m s)	( $^\circ$ ' '')	(mJy beam^-1)	(mJy)
VLA-A	1.3	$0.131 \times 0.095$	-13	0.06	18 34 40.284	-09 00 38.31	0.72	0.98
VLA-C	1.3	$1.1 \times 0.8$	0	0.05	...	...	1.31	1.44
VLA-A	3.6	$0.36 \times 0.24$	-5	0.03	...	...	0.47	0.59
VLA-C	3.6	$2.7 \times 1.9$	2	0.03	...	...	0.52	0.50

Notes. ^(a) The absolute position of the VLA-A 1.3 cm emission peak, obtained aligning positions of persistent water maser spots between the VLA and VLBA observations, should be accurate to about $\pm$ $0\hbox{$.\!\!^{\prime\prime}$ }01$ .

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