Low-frequency carbon radio recombination lines. I. Calculations of departure coefficients

Journal article

In the first paper of this series, we study the level population problem of recombining carbon ions. We focus our study on high quantum numbers, anticipating observations of carbon radio recombination lines to be carried out by the Low Frequency Array. We solve the level population equation including angular momentum levels with updated collision rates up to high principal quantum numbers. We derive departure coefficients by solving the level population equation in the hydrogenic approximation and including low-temperature dielectronic capture effects. Our results in the hydrogenic approximation agree well with those of previous works. When comparing our results including dielectronic capture, we find differences thatwe ascribe to updates in the atomic physics (e.g., collision rates) and to the approximate solution method of the statistical equilibrium equations adopted in previous studies. A comparison with observations is discussed in an accompanying article, as radiative transfer effects need to be considered.

Authors: Salgado, F; Morabito, L; Oonk, J; Salas, P; Toribio, M

• Publication status: Published
• Peer review status: Peer reviewed
• Publisher: Institute of Physics
• Journal: Astrophysical Journal
• Volume: 837
• Issue: 2
• Pages: 141
• Publication date: 2017-03-01
• Acceptance date: 2017-01-30
• DOI: 10.3847/1538-4357/aa5d9e
• EISSN: 1538-4357
• ISSN: 0004-637X
• Keywords: methods: numerical; ISM: general; ISM: atoms; line: formation; radio lines: ISM; radio lines: general