Table 1:
The characteristics of the selected pulsars taken from
Manchester et al. (2005). Period, P, distance, D,
spin-down age, spin-down luminosity,
,
and the corresponding
value for
,
and calculated magnetic field strength at the
neutron star surface,
,
and the light cylinder,
,
are listed. The last column shows the rank in
within the ATNF catalogue.
Pulsar name |
P |
D |
Age |
2*
 |
2*
 |
 |
 |
Rank |
PSR |
![$[\rm ms]$](/articles/aa/full/2007/17/aa6737-06/img27.gif) |
![$[\rm kpc]$](/articles/aa/full/2007/17/aa6737-06/img28.gif) |
![$[\rm kyears]$](/articles/aa/full/2007/17/aa6737-06/img29.gif) |
|
|
![$[\rm 10^{11}~G]$](/articles/aa/full/2007/17/aa6737-06/img30.gif) |
![$[\rm 10^4~G]$](/articles/aa/full/2007/17/aa6737-06/img31.gif) |
 |
B0531+21 |
J0534+2200 |
33.1 |
2 |
1.24 |
38.7 |
38.1 |
37.8 |
98.0 |
1 |
B0833-45 |
J0835-4510 |
89.3 |
0.29 |
11.3 |
36.8 |
37.9 |
33.8 |
4.45 |
2 |
B1706-44 |
J1709-4429 |
102 |
1.8 |
17.5 |
36.5 |
36.0 |
31.2 |
2.72 |
6 |
B1509-58 |
J1513-5908 |
151 |
4.4 |
1.55 |
37.3 |
36.0 |
154 |
4.22 |
7 |
|
J1747-2958 |
98.8 |
2.5 |
25.5 |
36.4 |
35.6 |
24.9 |
2.42 |
13 |
B1259-63 |
J1302-6350 |
47.8 |
1.5 |
332 |
35.9 |
35.5 |
3.3 |
2.87 |
15 |
|
J1811-1925 |
64.7 |
5 |
23.3 |
36.8 |
35.4 |
17.1 |
5.92 |
18 |
|
J1524-5625 |
78.2 |
3.8 |
31.8 |
36.5 |
35.3 |
17.7 |
3.46 |
19 |
|
J1420-6048 |
68.2 |
7.7 |
13 |
37.0 |
35.3 |
24.1 |
7.13 |
22 |
|
J1826-1334 |
101 |
4.1 |
21.4 |
36.4 |
35.2 |
27.9 |
2.51 |
23 |
|
J1801-2451 |
125 |
4.6 |
15.5 |
36.4 |
35.1 |
40.4 |
1.95 |
30 |
Source LaTeX |
All tables |
In the text