Table 2.
Open in new tab

Best-fitting parameters for the thermal radio emission models. The fits are based on observations at t ≳ 100–120 d in order to exclude contributions from the early radio peak.

NovaD|$v_{\rm min}^{(a)}$||$v_{\rm max}^{(b)}$|T(c)|$M_{\rm ej}^{(d)}$|Δt(e)
(kpc)(km s−1)(km s−1)(K)(M⊙)(d)
V1324 Sco7.855013001.2 × 1042.7 × 10−415
V1723 Aq6.127016001.0 × 1042.2 × 10−4−2.2
NovaD|$v_{\rm min}^{(a)}$||$v_{\rm max}^{(b)}$|T(c)|$M_{\rm ej}^{(d)}$|Δt(e)
(kpc)(km s−1)(km s−1)(K)(M⊙)(d)
V1324 Sco7.855013001.2 × 1042.7 × 10−415
V1723 Aq6.127016001.0 × 1042.2 × 10−4−2.2

Notes.(a)Minimum velocity.

(b)Maximum velocity.

(c)Ejecta temperature.

(d)Ejecta mass.

(e)Time delay between outflow ejection and optical outburst.

Table 2.
Open in new tab

Best-fitting parameters for the thermal radio emission models. The fits are based on observations at t ≳ 100–120 d in order to exclude contributions from the early radio peak.

NovaD|$v_{\rm min}^{(a)}$||$v_{\rm max}^{(b)}$|T(c)|$M_{\rm ej}^{(d)}$|Δt(e)
(kpc)(km s−1)(km s−1)(K)(M⊙)(d)
V1324 Sco7.855013001.2 × 1042.7 × 10−415
V1723 Aq6.127016001.0 × 1042.2 × 10−4−2.2
NovaD|$v_{\rm min}^{(a)}$||$v_{\rm max}^{(b)}$|T(c)|$M_{\rm ej}^{(d)}$|Δt(e)
(kpc)(km s−1)(km s−1)(K)(M⊙)(d)
V1324 Sco7.855013001.2 × 1042.7 × 10−415
V1723 Aq6.127016001.0 × 1042.2 × 10−4−2.2

Notes.(a)Minimum velocity.

(b)Maximum velocity.

(c)Ejecta temperature.

(d)Ejecta mass.

(e)Time delay between outflow ejection and optical outburst.

Close
This Feature Is Available To Subscribers Only

Sign In or Create an Account

Close

This PDF is available to Subscribers Only

View Article Abstract & Purchase Options

For full access to this pdf, sign in to an existing account, or purchase an annual subscription.

Close