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Very Long Baseline Interferometry Search for Nuclear Radio Continuum Emission in the Barred Spiral Galaxy NGC 7479

  • Authors: Seppo Laine, Emmanuel Momjian, Emilia Järvelä, Thomas P. Krichbaum, S. Komossa, Travis C. Fischer, Thomas G. Pannuti

Seppo Laine et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 2.

6 cm (left) and 18 cm (right) EVN images of the nuclear region of NGC 7479. The contour levels are at (–4, 4, 6, 8) × 16 μJy beam−1 (left) and at (–4, 4, 6, 8, 10, 12) × 17 μJy beam−1 (right). The synthesized beam sizes are 3.7 mas × 2.4 mas (P.A. = −7) and 14.1 mas × 9.2 mas (P.A. = 5) for the 6 and 18 cm images, respectively, and are shown in the lower left corner of each image. The grayscale wedges are in units of μJy beam−1. The letters “N” and “S” are used to label the components detected in the VLBA 6 cm image (Figure 3). Note that the nominal phase center of the observations is not in the center of the images in Figures 2 5.

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