Table 5.
Open in new tab

Derived pulsar kick velocity for the DEM S5 progenitor: estimated as a function of SNR age (Vpsr = 2 ×  dsmc × TAN(θ/2)/age) that simplifies to (θ ×  dsmc)/age since θ  |$\ll$| 1. The angular distance is θ = 73 arcsec. The adopted distance of dsmc = 67.5 kpc for the western side of the SMC is suggested by Scowcroft et al. (2016).

SNR age (kyr)|$V_{\rm psr\, at\, 60\, kpc}$| (km s−1)|$V_{\rm psr\, at\, 67.5\, kpc}$| (km s−1)
5.041574676
7.527713117
10.020782338
12.516631870
15.013861559
17.511881336
20.010391169
22.59241039
25.0831935
30.0693779
40.0520584
50.0416468
SNR age (kyr)|$V_{\rm psr\, at\, 60\, kpc}$| (km s−1)|$V_{\rm psr\, at\, 67.5\, kpc}$| (km s−1)
5.041574676
7.527713117
10.020782338
12.516631870
15.013861559
17.511881336
20.010391169
22.59241039
25.0831935
30.0693779
40.0520584
50.0416468
Table 5.
Open in new tab

Derived pulsar kick velocity for the DEM S5 progenitor: estimated as a function of SNR age (Vpsr = 2 ×  dsmc × TAN(θ/2)/age) that simplifies to (θ ×  dsmc)/age since θ  |$\ll$| 1. The angular distance is θ = 73 arcsec. The adopted distance of dsmc = 67.5 kpc for the western side of the SMC is suggested by Scowcroft et al. (2016).

SNR age (kyr)|$V_{\rm psr\, at\, 60\, kpc}$| (km s−1)|$V_{\rm psr\, at\, 67.5\, kpc}$| (km s−1)
5.041574676
7.527713117
10.020782338
12.516631870
15.013861559
17.511881336
20.010391169
22.59241039
25.0831935
30.0693779
40.0520584
50.0416468
SNR age (kyr)|$V_{\rm psr\, at\, 60\, kpc}$| (km s−1)|$V_{\rm psr\, at\, 67.5\, kpc}$| (km s−1)
5.041574676
7.527713117
10.020782338
12.516631870
15.013861559
17.511881336
20.010391169
22.59241039
25.0831935
30.0693779
40.0520584
50.0416468
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