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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 2.

The Raman-scattered O VI bands at 6825 Å (left) and 7082 Å (right) in Sanduleak’s star. The upper horizontal axis corresponds to the Doppler factor space ΔVatomic, whose origin has been chosen at the O VI line central wavelength in vacuum. The vertical bar in the left panel indicates the red bump and the three vertical bars in the right panel show the three peaks.

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