Open Access
Table 2
Parameters of the (double-)Maxwellians fitted to our results for the Verbunt et al. (2017) and Igoshev (2020) samples (fit), compared to the results from the corresponding literature (lit.), for young pulsars and the complete samples.
| Sample | Double-Maxwelliana | Maxwellianb | ||||
|---|---|---|---|---|---|---|
| σ1 [km/s] | σ2 [km/s] | w | σ [km/s] | |||
| Verbunt et al. | Young (τc ≤ 10 Myr) | fit | 96(1) | 382(6) | 0.31(1) | 331(13) |
| lit. | 82(27) | 328(53) | 0.32(16) | 273(33) | ||
| Complete | fit | 97(2) | 362(7) | 0.31(1) | 311(11) | |
| lit. | 75(17) | 316(47) | 0.42(13) | 239(24) | ||
| Igoshev | Young (τc ≤ 3 Myr) | fit | 46(1) | 307(6) | 0.20(1) | 309(11) |
| lit. | 56(10) | 336(45) | 0.20(11) | 295(34) | ||
| Complete | fit | 144(3) | 400(11) | 0.46(1) | 233(6) | |
| lit. | 128(20) | 298(28) | 0.42(16) | 225(18) | ||
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.