Figure 3 from A PROFILE ANALYSIS OF RAMAN-SCATTERED O VI BANDS AT 6825 Å AND 7082 Å IN SANDULEAK’S STAR

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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 3.

Schematic model of Sanduleak’s star. The O VI emission region is assumed to consist of an accretion disk, a bipolar outflow, and a further optically thick, compact component. See text for details.

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