Table 1
Pulsars associated with an SNR or PWN and with independent distance measurements.
| J2000 | B1950 | Distance | DMobs | DMNE2001 | Association | Refs. |
|---|---|---|---|---|---|---|
| (kpc) | (pc cm−3) | (pc cm−3) | ||||
| 0205+6449 | 2.0 ± 0.3 | 140.7 |  |
PWN 3C58 | 1 | |
| 0358+5413 (a) | 0355+54 |  |
57.1420 |  |
PWN | 2 |
| 0538+2817 | 1.3 ± 0.2 | 39.570 |  |
SNR S147 | 3 | |
| 0659+1414 | 0656+14 | 0.28 ± 0.03 | 14.0672 | 3.9 ± 0.5 | SNR Monogem Ring | 3 |
| 1016−5857 | 3 (b) | 394.2 |  |
PWN G284.3-1.8 | 4 | |
| 1124−5916 |  |
330 |  |
SNR G292.0+1.8 & PWN | 3 | |
| 1357−6429 | 2 − 2.5 ± 0.2 | 128.5 | 99.0(13.8) − 128.7(10.0)(c) | PWN | 5 | |
| 1400−6325 |  |
563 | 327.2(82.8) − 426.6(58.2)(c) | SNR G310.6-1.6 & PWN | 6, 7 | |
| 1550−5418 | 3.7 − 4.3 ± 0.3 | 830 | 183.7(41.4) − 245.3(37.6)(c) | SNR G327.24-0.13 | 8 | |
| 1709−4429 | 1706−44 |  |
75.69 |  |
PWN G343.1-2.3 | 3 |
| 1803−2137 (a) | 1800−21 |  |
233.99 |  |
SNR G8.7-0.1 & PWN | 3 |
| 1833−0827 | 1830−08 |  |
411 |  |
PWN | 3 |
| 1833−1034 | 4.1 ± 0.3 | 169.5 |  |
SNR G21.5-0.9 | 3 | |
| 1856+0113 (a) | 1853+01 | 2.5−2.6 ± 0.3 | 96.74 | 65.6(16.2) − 70.8(15.4)(c) | SNR & PWN W44 | 9 |
| 1907+0631 | 3.4 (a) | 428.6 |  |
SNR G40.5-0.5 | 10 | |
| 1930+1852 |  |
308 |  |
SNR & PWN G54.1+0.3 | 3 | |
| 1957+2831 | 9.2 − 10.2 ± 1(a) | 138.99 | 284(29.1) − 327.3(49.0)(c) | SNR G65.1+0.6 | 11 | |
| 2229+6114 | 0.8 (a) | 204.97 | 10.15 ± 1.9 | SNR G106.6+2.9 & PWN | 12 |
Notes. In case of multiple associations (from the ATNF catalog or other sources) the most recent work is cited. (a) For these sources a previous distance was included in the NE2001 model, but the remnant was not accounted for. (b) Distance error assumed to be 20% (10% on H I). (c) These DMs are determined from H I distance measurements and while these errors are symmetric, when translating to DM errors, they are asymmetric. Consequently, the respective errors are given for the corresponding bounds.
References.(1) Kothes (2013); (2) Chatterjee et al. (2004); (3) Verbiest et al. (2012); (4) Camilo et al. (2004); (5) Danilenko et al. (2012); (6) Renaud et al. (2010); (7) Marshall et al. (2006); (8) Gelfand & Gaensler (2007); (9) Cox et al. (1999); (10) Yang et al. (2006); (11) Tian & Leahy (2006); (12) Kothes et al. (2001).
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