text:   hydrodynamics/radiative approach",1,"[""Today we release 'Introducing the HD+B model for pulsar wind nebulae: a hybrid hydrodynamics/radiative approach', MNRAS @RoyalAstroSoc, <LINK>. This is a novel method to study pulsar wind nebulae. A hopefully intuitive conceptual summary is shown in the figure. <LINK>""]",20,04,268