Table 2.
Selected known magnetars and their properties.
| Magnetar | B [×1014 G] | D [kpc] | Lpeak [×1038 erg s−1] | ||||
|---|---|---|---|---|---|---|---|
| APR | ENG | H4 | SLy | WFF | |||
| SGR 1806−20 | 19.6 | 8.7 | 15.3 | 18.0 | 28.5 | 17.2 | 12.9 |
| 1E 1841−045 | 7.03 | 8.5 | 3.29 | 3.87 | 8.75 | 3.55 | 2.69 |
| SGR 1900+14 | 7.00 | 12.5 | 3.27 | 3.82 | 8.72 | 3.55 | 2.67 |
| SGR 0526−66 | 5.60 | 53.6 | 2.69 | 3.07 | 5.12 | 2.95 | 2.13 |
| CXOU J171405.7−381031 | 5.01 | 10.2 | 2.28 | 2.68 | 3.64 | 2.47 | 1.74 |
| 1RXS J170849.0−400910 | 4.68 | 3.8 | 2.08 | 2.42 | 3.32 | 2.27 | 1.57 |
| CXOU J010043.1−721134 | 3.93 | 62.4 | 1.47 | 1.85 | 2.70 | 1.72 | 0.97 |
| Swift J1818.0−1607 | 3.54 | 4.8 | 1.14 | 1.51 | 2.38 | 1.33 | 0.85 |
| PSR J1622−4950 | 2.74 | 9.0 | 0.84 | 0.99 | 1.48 | 0.92 | 0.67 |
| SGR J1745−2900 | 2.31 | 8.3 | 0.71 | 0.83 | 1.22 | 0.78 | 0.49 |
| XTE J1810−197 | 2.10 | 3.5 | 0.60 | 0.75 | 1.10 | 0.69 | 0.33 |
| SGR 0501+4516 | 1.87 | 2.0 | – | – | – | – | – |
| Swift J1834.9−0846 | 1.42 | 4.2 | – | – | – | – | – |
| 4U 0142+61 | 1.34 | 3.6 | – | – | – | – | – |
| Swift J1822.3−1606 | 0.14 | 1.6 | – | – | – | – | – |
| SGR 0418+5729 | 0.06 | 2.0 | – | – | – | – | – |
Notes. For each EOS, we assumed a fixed magnetar mass of 1.4 M⊙ when computing the peak bolometric luminosity Lpeak. Magnetars with a total ejecta mass of Mej < 10−9 M⊙ were not considered, as such small ejecta masses are unlikely to support significant nucleosynthesis during a nova brevis event.
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.