B1839-04 at 1.4 GHz
This table is automatically generated. See
this page
for an explanation of table entries.
Source
RA (J2000)
Dec (J2000)
Flux (mJy)
RMS (mJy)
D(')
Comments
Image
B1839-04.001
18 42 26.45062
-03 59 59.1501
7.1
0.40
0.00
Pulsar
B1839-04.002a
18 42 58.10115
-04 13 56.5191
5.1
0.26
16.03
Top source -- extended
B1839-04.002b
18 42 58.11609
-04 14 04.0449
5.2
0.26
16.14
Bottom source - extended
B1839-04.003
18 43 14.58228
-03 59 06.0671
5.0
0.21
12.04
Extended
B1839-04.004a
18 43 03.49609
-04 00 12.6413
7.9
0.30
9.24
Center source -- pointlike?
B1839-04.004b
18 43 04.47714
-04 00 14.0529
2.3
0.30
9.49
Left source -- pointlike?
B1839-04.005
18 43 28.45497
-03 50 18.5696
4.5
0.19
18.24
Extended
B1839-04.006
18 43 31.37294
-03 47 43.5544
2.8
0.30
20.31
Extended
B1839-04.007
18 41 27.28687
-03 48 43.6949
15.2
0.19
18.56
BW smeared -- pointlike?
B1839-04.008
18 42 58.66035
-03 53 06.1219
3.2
0.28
10.58
Extended
B1839-04.009
18 42 49.49155
-04 09 47.6540
2.3
0.26
11.37
Hugely extended
B1839-04.011
18 42 15.05352
-03 43 59.6719
1.3
0.24
16.24
Extended
B1839-04.012
18 41 42.50431
-03 49 54.4545
2.6
0.24
14.89
Slightly extended? Weak
Return to
the main VLA Survey page
.
Shami Chatterjee
shami@astro.cornell.edu
Auto generated: Thu Mar 21 15:58:05 2002