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Arp 220: New Observational Insights into the Structure and Kinematics of the Nuclear Molecular Disks and Surrounding Gas

  • Authors: Jordan Wheeler, Jason Glenn, Naseem Rangwala, and Adalyn Fyhrie

2020 The Astrophysical Journal 896 43.

  • Provider: AAS Journals

Caption: Figure 11.

Models for the Arp 220 eastern nucleus in 12CO J = 3–2 (orange lines) and 13CO J = 4–3 (purple lines) shown along with the observed line profiles at half-beam increments along the disk axis and perpendicular to the disk axis. The column density of the model in the central position is 1.3 × 1025 H2 cm−2 for 12CO and 3.3 × 1024 H2 cm−2 for 13CO. Moving either to the left or right one panel at a time, the models’ column density decreases to 8.3 × 1024 H2 cm−2, 4.2 × 1024 H2 cm−2, and 2.0 × 1024 H2cm −2 for 12CO and to 2.2 × 1024 H2 cm−2, 1.2 × 1024 H2 cm−2, and 6.5 × 1023 H2 cm−2 for 13CO. Likewise, moving one panel at time in the vertical direction, the column density decreases to 2.9 × 1024 H2 cm−2 and 3.1 × 1023 H2 cm−2 for 12CO and to 9.3 × 1023 H2 cm−2 and 1.4 × 1023 H2 cm−2 for 13CO. For 12CO J = 3 → 2, 1 Jy/beam = 248 K, and for 13CO J = 4 → 3, 1 Jy/beam = 294.5 K. An interactive figure is available.

An interactive version of this figure is available in the online journal.

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