Spectral line profiles changed by dust scattering in heavily obscured young stellar objects

TL;DR

This paper investigates how dust scattering affects spectral line profiles in heavily obscured young stellar objects, proposing a remote scattering approximation to model these effects and analyzing resulting line profile changes.

Contribution

It introduces a remote scattering approximation method to calculate spectral line profiles influenced by circumstellar dust in young stellar objects.

Findings

Dust scattering significantly alters line profiles in obscured young stars.

The method models both stationary and moving dust effects on spectral lines.

Results demonstrate the impact of dust motion on H alpha line profiles.

Abstract

It is known that scattering of radiation by circumstellar dust can strongly change the line profiles in stellar spectra. This hampers the analysis of spectral lines originating in the emitting regions of heavily obscured young stars. To calculate the line profile of the scattered radiation, we suggest to use the approximation of remote scattering particles. This approximation assumes that the scattering dust grains are at a distance from the star that is much larger than the characteristic size of the emitting region. Using this method, we calculated the line profiles of several simple models. They show the H alpha line profiles of Herbig AeBe stars in the presence and absence of motionless or moving dust.