text:   emission and mass accretion rate in massive young stellar objects",1,"['CO overtone emission is a really useful tracer of small-scale discs around massive YSOs, but why do we only see it in ~25% of spectra? \n\nManfred Mann said it best - we’re just blinded by the light. \n\nNew paper out now: <LINK>\n\n#Astronomy #Arxiv #Astroph 😎 <LINK>']",18,04,259