Table 3 Updated values of density of the shocked interstellar medium from previous XMM-Newton data analysis29
From: The supernova remnant SN 1006 as a Galactic particle accelerator
Azimuthal opening angle (∘) | Region name29 | Density (cm−3) |
---|---|---|
53–63 | a | \(0.20{6}_{-0.13}^{+0.2}\) |
58–73 | b | \(0.19{7}_{-0.08}^{+0.05}\) |
65–80 | c | \(0.18{9}_{-0.07}^{+0.05}\) |
73–88 | d | \(0.16{9}_{-0.08}^{+0.03}\) |
80–96 | e | \(0.15{0}_{-0.06}^{+0.05}\) |
88–103 | f | \(0.15{2}_{-0.08}^{+0.07}\) |
96–112 | g | \(0.19{9}_{-0.11}^{+0.09}\) |
104–120 | h | \(0.20{1}_{-0.11}^{+0.09}\) |