# Publications

### The physical origins and dominant emission mechanisms of Lyman-alpha halos: results from TNG50 in comparison to MUSE observations

Extended Lyman-alpha emission around galaxies and quasars at high redshift – Lyman-alpha halos (LAHs) – are now commonly …

### Variations of Observed Lyman-α Spectra Shapes due to the Intergalactic Absorption

Lyman-$\alpha$ (Ly$\alpha$) spectra provide insights into the small-scale structure and kinematics of neutral hydrogen (HI) within …

### Radiative Transfer Distortions of Lyman-α Emitters: a New Fingers-of-God Damping in the Clustering in Redshift Space

Complex radiative transfer (RT) of the Lyman-$\alpha$ photons poses a theoretical challenge to galaxy surveys which infer the …

### The Intrinsic Stochasticity of the $^{56}$Ni Distribution of Single-Degenerate Near-Chandrasekhar Mass Type Ia Supernovae

Chandrasekhar-mass white dwarfs accreting mass from non-degenerate stellar companions through the single-degenerate channel have …

### The impact of Lyman-α radiative transfer on large-scale clustering in the Illustris simulation

Lyman-$\alpha$ emitters (LAEs) are a promising probe of the large-scale structure at high redshift, $z\gtrsim 2$. In particular, the …

### Viscosity, pressure, and support of the gas in simulations of merging cool-core clusters

Major mergers are considered to be a significant source of turbulence in clusters. We performed a numerical simulation of a major …

### Constraining The Single-Degenerate Channel of Type Ia Supernovae With Stable Iron-Group Elements in SNR 3C 397

Recent Suzaku X-ray spectra of SNR 3C 397 indicate enhanced stable iron-group element abundances of Ni, Mn, Cr, and Fe. Seeking to …