LENSEDQUASAR
4C–05.55, NRAO 41
 
 
3C 279
12ʰ 56ᴹ 11.1ˢ
0.5362 ± 0.0004
Ṯhe problem with viscosity﹍﹍
luminosities close to the Eddington luminosity (∽1046⁴⁶ erg s⁻¹ for a typical ~10⁸ M⊙ SMBH masses) produced﹏﹏the regular, line driven stellar winds can only stand for a mass loss rate of around 10⁻⁴–10⁻³ solar masses per year