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UV and Hα HST Observations of Six GASP Jellyfish Galaxies

  • Authors: Marco Gullieuszik, Eric Giunchi, Bianca M. Poggianti, Alessia Moretti, Claudia Scarlata, Daniela Calzetti, Ariel Werle, Anita Zanella, Mario Radovich, Callum Bellhouse, Daniela Bettoni, Andrea Franchetto, Jacopo Fritz, Yara L. Jaffé, Sean L. McGee, Matilde Mingozzi, Alessandro Omizzolo, Stephanie Tonnesen, Marc Verheijen, Benedetta Vulcani

Marco Gullieuszik et al 2023 The Astrophysical Journal 945 .

  • Provider: AAS Journals

Caption: Figure 7.

Zoom of the F275W and Hα images of JO201 (left panels) and JO206 (right panels) on two SF regions; their position is marked by the green squares in the top panels. The blue and red lines are isophotes of the F275W and Hα emission, respectively, which are overplotted to highlight the differences in the spatial distribution of Hα and UV emission. The arrows in the central panels suggest the approximate direction of the ram pressure wind.

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