Upper Limits to Magnetic Fields in the Outskirts of Galaxies

• Main Authors: Ericson López, Jairo Armijos-Abendaño, Mario Llerena, Franklin Aldás
• Format: Article
• Language: English
• Published: MDPI AG 2017-09-01
• Series: Galaxies
• Subjects: nearby galaxies; magnetic fields; molecules
• Online Access: https://www.mdpi.com/2075-4434/5/3/55

Based on CO(2-1) public data, we study the monoxide oxygen gas excitation conditions and the magnetic field strength of four spiral galaxies. For the galaxy outskirts, we found kinetic temperatures in the range of ≲35–38 K, CO column densities ≲ 10 15 – 10 16 cm - 2 , and H 2 masses ≲ 4 × 10 6 – 6 × 10 8 M ⊙ . An H 2 density ≲ 10 3 cm - 3 is suitable to explain the 2 σ upper limits of the CO(2-1) line intensity. We constrain the magnetic field strength for our sample of spiral galaxies and their outskirts by using their masses and H 2 densities to evaluate a simplified magneto-hydrodynamic equation. Our estimations provide values for the magnetic field strength on the order of ≲6–31 μ G.