TY - JOUR

T1 - Spectral line profiles changed by dust scattering in heavily obscured young stellar objects

AU - Grinin, V. P.

AU - Tambovtseva, L. V.

AU - Weigelt, G.

PY - 2012

Y1 - 2012

N2 - 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 Hα line profiles of Herbig AeBe stars in the presence and absence of motionless or moving dust.

AB - 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 Hα line profiles of Herbig AeBe stars in the presence and absence of motionless or moving dust.

KW - Line: profiles

KW - Scattering

KW - Stars: pre-main sequence

KW - Stars: winds, outflows

UR - http://www.scopus.com/inward/record.url?scp=84864253649&partnerID=8YFLogxK

U2 - 10.1051/0004-6361/201219768

DO - 10.1051/0004-6361/201219768

M3 - Article

AN - SCOPUS:84864253649

VL - 544

JO - ASTRONOMY & ASTROPHYSICS

JF - ASTRONOMY & ASTROPHYSICS

SN - 0004-6361

M1 - A45

ER -