Modelling CHOH masers: Sobolev approximation and accelerated lambda iteration method
arXiv:1511.07188 · doi:10.1093/mnras/stv2594
Abstract
A simple one-dimensional model of CHOH maser is considered. Two techniques are used for the calculation of molecule level populations: the accelerated lambda iteration (ALI) method and the large velocity gradient (LVG), or Sobolev, approximation. The LVG approximation gives accurate results provided that the characteristic dimensions of the medium are larger than 5-10 lengths of the resonance region. We presume that this condition can be satisfied only for the largest observed maser spot distributions. Factors controlling the pumping of class I and class II methanol masers are considered.
9 pages, 5 figures; accepted for publication in MNRAS
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- Modelling cosmic masers in C-type shock waves -- the coexistence of Class I CH3OH and 1720 MHz OH masers
- Collisional Pumping of OH Masers near Supernova Remnants
- An nl-model with radiative transfer for hydrogen recombination line masers
- The Sobolev approximation for radiation transport with line overlap and continuous opacity
- A 95 GHz Methanol Emission Survey Toward Eight Small Supernova Remnants
- Collisional Pumping of HO and CHOH Masers in C-Type Shock Waves
- An nl-model with a full radiative transfer treatment for level populations of hydrogen atoms in a spherically symmetric H II region