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Mapping the Filamentary Nebula of NGC 1275 with Multiwavelength SITELLE Observations

  • Authors: Carter Lee Rhea, Julie Hlavacek-Larrondo, Marie-Lou Gendron-Marsolais, Benjamin Vigneron, Megan Donahue, Auriane Thilloy, Laurie Rousseau-Nepton, Mar Mezcua, Norbert Werner, Jorge Barrera-Ballesteros, Hyunseop Choi, Alastair Edge, Andrew Fabian, G. Mark Voit

Carter Lee Rhea et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 9.

The left panel is a diagram of the shock region in NGC 1275. The background image is the Chandra soft X-ray emission between 0.5 and 2.0 keV described in Section 2.2; the contours highlight the Hα emission. We highlight the location of the shock front (blue) as detected in A. C. Fabian & J. S. Sanders (2006). In the right-hand panel, we show the WHAN plot for the bar in the shock region (orange) and the small northern filament (green) that has not yet gone through the shock.

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