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A PROFILE ANALYSIS OF RAMAN-SCATTERED O VI BANDS AT 6825 Å AND 7082 Å IN SANDULEAK’S STAR

  • Authors: Jeong-Eun Heo, Rodolfo Angeloni, Francesco Di Mille, Tali Palma, and Hee-Won Lee

2016 The Astrophysical Journal 833 286.

  • Provider: AAS Journals

Caption: Figure 5.

Monte Carlo simulations of Raman-scattered O VI λλ 1032 (left panel) and 1038 (right panel) for various NH I. The solid line shows the observation, while the dotted lines represent the results of our Monte Carlo simulations.

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