Table 4.

Best-fitting parameters of synchrotron model.

Nova|$v_1^{(a)}$||$v_4^{(b)}$||$n_{4}/n_{1}^{(c)}$||$\tilde{v}_{\rm f}^{(d)}$|Δt(e)H(f)n0(g)ϵe(h)fEUV(i)
(km s−1)(km s−1)(km s−1)(d)(cm)(cm−3)
V1324 Sco17006700.43630123.7 × 10137.8 × 1090.0810.051
V1723 Aql23007700.668303.29.5 × 10136.7 × 1070.0150.31
V5589 Sgr22001902.381056.8 × 10134.1 × 1080.0140.07
Nova|$v_1^{(a)}$||$v_4^{(b)}$||$n_{4}/n_{1}^{(c)}$||$\tilde{v}_{\rm f}^{(d)}$|Δt(e)H(f)n0(g)ϵe(h)fEUV(i)
(km s−1)(km s−1)(km s−1)(d)(cm)(cm−3)
V1324 Sco17006700.43630123.7 × 10137.8 × 1090.0810.051
V1723 Aql23007700.668303.29.5 × 10136.7 × 1070.0150.31
V5589 Sgr22001902.381056.8 × 10134.1 × 1080.0140.07

Notes.(a)Velocity of fast outflow.

(b)Velocity of slow outflow (DES).

(c)Ratio of densities of DES and fast outflow.

(d)Velocity of the shock in the frame of the upstream gas, calculated from v1, v4, n4/n1 using equation (3).

(e)Time delay between launching fast and slow outflows.

(f)Scaleheight of slow outflow.

(g)Normalization of density profile of slow outflow (equation 7).

(h)Fraction of shock power placed into power-law relativistic electrons/positrons.

(i)Fraction of shock power placed into hydrogen-ionizing radiation (equation 5).

Table 4.

Best-fitting parameters of synchrotron model.

Nova|$v_1^{(a)}$||$v_4^{(b)}$||$n_{4}/n_{1}^{(c)}$||$\tilde{v}_{\rm f}^{(d)}$|Δt(e)H(f)n0(g)ϵe(h)fEUV(i)
(km s−1)(km s−1)(km s−1)(d)(cm)(cm−3)
V1324 Sco17006700.43630123.7 × 10137.8 × 1090.0810.051
V1723 Aql23007700.668303.29.5 × 10136.7 × 1070.0150.31
V5589 Sgr22001902.381056.8 × 10134.1 × 1080.0140.07
Nova|$v_1^{(a)}$||$v_4^{(b)}$||$n_{4}/n_{1}^{(c)}$||$\tilde{v}_{\rm f}^{(d)}$|Δt(e)H(f)n0(g)ϵe(h)fEUV(i)
(km s−1)(km s−1)(km s−1)(d)(cm)(cm−3)
V1324 Sco17006700.43630123.7 × 10137.8 × 1090.0810.051
V1723 Aql23007700.668303.29.5 × 10136.7 × 1070.0150.31
V5589 Sgr22001902.381056.8 × 10134.1 × 1080.0140.07

Notes.(a)Velocity of fast outflow.

(b)Velocity of slow outflow (DES).

(c)Ratio of densities of DES and fast outflow.

(d)Velocity of the shock in the frame of the upstream gas, calculated from v1, v4, n4/n1 using equation (3).

(e)Time delay between launching fast and slow outflows.

(f)Scaleheight of slow outflow.

(g)Normalization of density profile of slow outflow (equation 7).

(h)Fraction of shock power placed into power-law relativistic electrons/positrons.

(i)Fraction of shock power placed into hydrogen-ionizing radiation (equation 5).

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