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High-resolution Giant Metrewave Radio Telescope H I 21 cm Imaging of the Host Galaxy of FRB 20250316A

  • Authors: Balpreet Kaur, Nissim Kanekar, J. Xavier Prochaska

Balpreet Kaur et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 3.

GMRT H I 21 cm velocity moment images of NGC 4141 at an angular resolution of ﹩10\mathop{.}\limits^{^{\prime\prime} }0﹩. (A) The velocity-integrated moment-0 image, on a color scale and using contours. The lowest contour is at the 3σ H I column density sensitivi of the spectral cube, 1.3 × 1020 cm−2 per 10.4 km s−1, with subsequent contours increasing in steps of 3.5 × 1020 cm−2 (i.e., 8σ); the highest H I column density contour is at 3.2 × 1021 cm−2. (B) The moment-0 image of (A) (contours), overlaid on the DECaLS g-band image (color scale; A. Dey et al. 2019). (C) The H I 21 cm velocity field; the velocity contours are at intervals of 15 km s−1, with negative velocities indicated by dashed contours. (D) The H I 21 cm velocity dispersion map; the contours are at intervals of 10 km s−1. In all panels, the axes are relative to the center of NGC 4141, with the magenta star indicating the location of FRB 20250316A, and the gray circle in the inset at the bottom left indicating the GMRT synthesized beam.

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