Figure 16 from Probing for Exoplanets Hiding in Dusty Debris Disks: Disk Imaging, Characterization, and Exploration with HST/STIS Multi-roll Coronagraphy

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Probing for Exoplanets Hiding in Dusty Debris Disks: Disk Imaging, Characterization, and Exploration with HST/STIS Multi-roll Coronagraphy

Authors: Glenn Schneider, Carol A. Grady, Dean C. Hines, Christopher C. Stark, John H. Debes, Joe Carson, Marc J. Kuchner, Marshall D. Perrin, Alycia J. Weinberger, John P. Wisniewski, Murray D. Silverstone, Hannah Jang-Condell, Thomas Henning, Bruce E. Woodgate, Eugene Serabyn, Amaya Moro-Martin, Motohide Tamura, Phillip M. Hinz, and Timothy J. Rodigas

Schneider et al. 2014 The Astronomical Journal 148 59.

Provider: AAS Journals

Caption: Figure 16.

V05 − V06 difference image of the HD 32297 CS disk, differentially rolled by the planned, nominal, 30° with the star occulted at the 0 farcs 6 wide WedgeA occulter position in both orientations. In the regions where the positive and negative imprints of the disk flux do not overlap, this and similar other paired images inform us that the sensible disk flux originates only to the NW side of the star and within no more than 0 farcs 2 (narrower than the half-width of the WedgeA-0.6 occulter) to the SW of the plane of the edge-on disk.

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