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Table 3

Characteristics of nearby SNRs, from Delahaye et al. (2010).

SNR Other name Distance Age
G+long+lat [kpc] [kyr]

18.95–1.1 2.0 ± 0.1 11.75 ± 0.85
65.3+5.7 0.9 ± 0.1 26 ± 1
65.7+1.2 DA 495 1.0 ± 0.4 16.75 ± 3.25
69.0+2.7 CTB 80 2.0 ± 0.1 20 ± 1
74.0–8.5 Cygnus Loop 10 ± 1
78.2+2.1 γ Cygni 1.5 ± 0.1 7 ± 1
82.2+5.3 W63 2.3 ± 1.0 20.1 ± 6.6
89.0+4.7 HB 21 1.7 ± 0.5 5.60 ± 0.28
93.7–0.2 CTB 104A 1.5 ± 0.2 50 ± 20
114.3+0.3 0.7 7.7 ± 0.1
116.5+1.1 1.6 20 ± 5
116.9+0.2 CTB 1 1.6 20 ± 5
119.5+10.2 CTA 1 1.4 ± 0.3 10 ± 5
127.1+0.5 R5 1.0 ± 0.1 25 ± 5
156.2+5.7 0.8 ± 0.5 10 ± 1
160.9+2.6 HB 9 0.8 ± 0.4 5.5 ± 1.5
180.0–1.7 S147 1.2 ± 0.4 600 ± 10
184.6–5.8 Crab nebula 2.0 ± 0.5 7.5
189.1+3.0 IC 443 1.5 ± 0.1 30 or 4
203.0+12.0 Monogem ring 86 ± 1
205.5+0.5 Monoceros Nebula 1.63 ± 0.25 29 ± 1
263.9–3.3 Vela(XYZ) 0.295 ± 0.075 11.2 ± 0.1
266.2–1.2 Vela Jr 0.75 ± 0.01 3.5 ± 0.8
276.5+19.0 Antlia 0.2 ± 0.14  ≥  1,000
315.1+2.7 1.7 ± 0.8 50 ± 10
330.0+15.0 Lupus Loop 1.2 ± 0.3 50 ± 10
347.3–0.5 SN393 1.0 ± 0.3 4.9

Notes. See the original paper for a discussion of the errors and for more extensive information.

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