Parameters for the models used in this study as well as the injected power obtained by matching the calculated flux with the observed one.
|Model||L (kpc)||D0 (kpc2 Myr−1)||δ||Vwind (km s−1)||vA(km s−1)||α||𝒫inj|
|MIN2.4||1.0||0.0016||0.85||13.5||22.4||2.4||2.9 × 1045|
|MED2.2||4.0||0.012||0.7||12.0||52.9||2.2||3.2 × 1041|
|MED2.3||2.3||4.3 × 1041|
|MED2.4||2.4||6.5 × 1041|
|MAX2.2||15.0||0.0765||0.46||5.0||117.6||2.2||6.9 × 1040|
|MAX2.3||2.3||9.2 × 1040|
|MAX2.4||2.4||1.4 × 1041|
|*Kr2.4||10||0.09||0.5||10.0||28.0||2.4||2.8 × 1041|
|*Kol2.55||10||0.23||1/3||12.0||30.0||2.55||6 × 1041|
Notes. The number appearing in the name of the model corresponds to the value of the logarithmic exponent α in the source term. (*)Models with a star are described in Sect. 4.2 and reproduce the observed primary fluxes.
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