Ly$\alpha$ Spectra from Multiphase Outflows, and their Connection to Shell Models
Max Gronke, Mark Dijkstra

TL;DR
This study uses Monte Carlo simulations to analyze how multiphase outflow properties influence Ly$ ext{alpha}$ spectra and compares these with shell models, revealing key physical parameters shaping the spectra.
Contribution
It provides a comprehensive analysis of Ly$ ext{alpha}$ spectra from multiphase outflows and explores the connection and limitations of shell models in representing these complex media.
Findings
Cloud covering factor significantly influences spectra.
Residual HI in hot medium affects spectral shape.
Shell model parameters often do not match physical properties of multiphase media.
Abstract
We perform Lyman- (Ly) Monte-Carlo radiative transfer calculations on a suite of models of multiphase, outflowing media, which are characterized by parameters. We focus on the Ly spectra emerging from these media, and investigate which properties are dominant in shaping the emerging Ly profile. Multiphase models give rise to a wide variety of emerging spectra, including single, double and triple peaked spectra. We find that the dominant parameters in shaping the spectra include (i) the cloud covering factor, , in agreement with earlier studies, and (ii) the temperature and number density of residual HI in the hot ionized medium. We attempt to reproduce spectra emerging from multiphase models with `shell models' which are commonly used to fit observed Ly spectra, and investigate the connection between shell-model parameters and the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
