Raman-Scattered Balmer Wings in Symbiotic Stars

  • 이희원 (세종대학교 천문우주학과)
  • Published : 2011.10.05

Abstract

Many symbiotic stars exhibit features formed through Raman scattering with hydrogent atom, which can be useful in probing the mass loss and mass transfer processes. These include Raman scattered O VI 6830, 7088, Raman scattered He II 6545, 4850, 4332, and broad wings around Balmer emission lines. In this study we investigate the basic properties of broad Balmer wings formed through Raman scattering using a Monte Carlo technique. Special attention is made on the symmetry of the wings which is expected to be broken due to asymmetric scattering cross section. In this poster, we show preliminary results.

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