We have used the Very Large Array to search for compact milliarcsecond-size radio sources near methanol masers in high-mass star-forming regions. Such sources are required for Very Long Baseline Interferometry phase-referencing observations. We conducted p
21 55 50
060831+215535
45
40
)
0002J( N35
OITANILCE30
D25
20
15
06 08 32.5
32.0
31.531.0
30.5
30.0
RIGHT ASCENSION (J2000)
C array
21 34 25
061026+21341220
)
00015
2J( NOITA10
NILCED05
0033 55
06 10 28.027.5
27.026.526.025.5RIGHT ASCENSION (J2000)
-17 17 15
072912 171729
20
25
)
0002J( N30
OITANILC35
ED40
45
50
07 29 13.0
12.512.011.5
11.0
RIGHT ASCENSION (J2000)
C array-16 28 50
073002 162904
55
)
029 00
002J( NO05
ITANILCE10
D15
20
25
07 30 04.0
03.5
03.0
02.502.0
01.5
01.0
RIGHT ASCENSION (J2000)
22 30 00J0608+2229
29 55
50
)
000245
J( NOITAN40
ILCED35
30
25
06 08 35.5
35.0
34.534.0
33.5
33.0
RIGHT ASCENSION (J2000)
C array
-16 48 10
072833 16482515
20
)
0002J25( NOITAN30ILCED35
40
45
07 28 35.034.5
34.033.5
33.032.5RIGHT ASCENSION (J2000)
-16 36 40
072924 163656
45
50
)
0002J(55
NOITANIL37 00
CED05
10
15
07 29 25.0
24.5
24.023.5
23.0
RIGHT ASCENSION (J2000)
C array-16 32 05
073111 163223
10
15
)
000220
J( NOITA25
NILCED30
35
40
45
07 31 12.5
12.0
11.511.0
10.5
10.0
RIGHT ASCENSION (J2000)
22 29 48
J0608+2229
46
)
044
002J( NOITA42
NILCED40
38
36
06 08 34.8
34.7
34.6
34.5
34.434.334.234.134.0
33.9
RIGHT ASCENSION (J2000)
C array
-17 29 45
072858 173000
50
55
)
0002J30 00
( NOITANI05
LCED10
15
20
07 28 59.559.0
58.558.057.557.0
RIGHT ASCENSION (J2000)
-16 36 53
072924 163656
54
55
)
0002J56
( NOITAN57
ILCED58
59
37 00
01
07 29 24.2
24.1
24.023.923.823.7
RIGHT ASCENSION (J2000)
C array-16 32 18
073111 163223
20
)
0002J22
( NOITANILC24
ED26
28
07 31 11.8
11.7
11.6
11.511.411.311.211.1
11.0
RIGHT ASCENSION (J2000)