The physics of water masers observable with ALMA and SOFIA: model predictions for evolved stars

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	374-404
Number of pages	31
Journal	Monthly Notices of the Royal Astronomical Society
Volume	456
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stv2437
Publication status	Published - 11 Feb 2016

masers-radiation mechanisms, general-radiative transfer-techniques, high angular resolution-ISM, lines and bands-radio lines, general, YOUNG STELLAR OBJECTS, VY-CANIS-MAJORIS, OPACITY-SAMPLING MODELS, GIANT BRANCH STARS, H2O MASER, FORMING REGIONS, CIRCUMSTELLAR ENVELOPES, MIRA VARIABLES, RADIATIVE-TRANSFER, SPECTRAL-LINE

ID: 662136