We present a basic model for the calculation of the luminosity distribution of supernova remnant populations. We construct theoretical Ha and joint [S II] - Ha luminosity functions for supernova remnants by combining prescriptions from a basic evolution model that provides the shock velocity and radius for SNRs of different age and pre-shock density, with shock excitation models that give the gas emissivity for shocks of different physical parameters. We assume a flat age distribution, and we explore the effect of different pre-shock density distributions or different magnetic parameters. We find very good agreement between the shape of the model Ha and the joint [S II] - Ha luminosity functions and those measured from SNR surveys in nearby galaxies.
@article{arxiv.2205.09130,
title = {Optical emission-line Luminosity Function models for populations of Supernova Remnants},
author = {M. Kopsacheili and A. Zezas and I. Leonidaki},
journal= {arXiv preprint arXiv:2205.09130},
year = {2022}
}