Table 2
Determined values of the phase lag between the peak (or midpoint) of the pulse profile and the inflexion of the PA profile, Δφ, shown in degrees in Col. 2, for 11 pulsars observed at 150 MHz.
| PSR | Δφ [deg] | rem [km] | RLC [km] |
|
|
|||
| B0809+74 | 10 |
– | 61, 657 |
| B0823+26 | 1 |
144 |
25, 320 |
| B0834+06 | 2 |
452 |
60, 776 |
| B0950+08 | 0 |
– | 12, 075 |
| J1022+1001 | −2 |
– | 785 |
| B1133+16 | 1.4 |
349 |
56, 679 |
| B1508+55 | −1.9 |
– | 35, 293 |
| B1919+21 | 2 |
– | 63, 807 |
| B1929+10 | −10 |
– | 10, 808 |
| B1953+50 | 1.6 |
177 |
24, 760 |
| B2224+65 | 2 |
– | 32, 566 |
Notes. For four pulsars, for which the peak (or midpoint) of the profile precedes the PA inflexion within the quoted 1σ uncertainties, Col. 3 shows the emission height, rem, calculated in the framework of BCW (Eq. (10)). For the rest of the pulsars, Δφ is negative within 1σ or its sign cannot be confidently determined; therefore, an emission height was not calculated for those pulsars. Column 4 shows the light-cylinder radius, RLC, of each pulsar, in km.
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