Simulation of pumping mechanism of H2O-masers in circumstellar envelopes of late-type stars
Author:
Publisher
IOP Publishing
Subject
General Physics and Astronomy
Link
http://stacks.iop.org/1742-6596/461/i=1/a=012009/pdf
Reference13 articles.
1. Evolved star water maser cloud size determined by star size
2. Numerical methods for non-LTE line radiative transfer: Performance and convergence characteristics
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2. The physics of water masers observable with ALMA and SOFIA: model predictions for evolved stars;Monthly Notices of the Royal Astronomical Society;2015-12-14
3. Modelling CH3OH masers: Sobolev approximation and accelerated lambda iteration method;Monthly Notices of the Royal Astronomical Society;2015-12-03
4. Model of the vibrationally excited H2O maser at 658 GHz in circumstellar envelopes around asymptotic giant branch stars;Monthly Notices of the Royal Astronomical Society;2015-04-03
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