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Open Access PaperThis journal vol. entitled: 11th Pacific Rim Conference on Stellar Astrophysics: Physics and Chemistry of the Late Stages of Stellar Evolution, 14–17 December 2015, Hong Kong, PR ChinaConference Theme: Physics and Chemistry of  the Late Stages of Stellar EvolutionThe transitional phase between the asymptotic giant branch (AGB) and post-AGB phases holds the key to our understanding of the late-stage metamorphosis of intermediate-mass stars. Here we briefly report the results of our latest OH and H2O maser surveys in which a new WF candidate (IRAS 19356+0754) was found. We also performed radiative transfer modelling on the spectral energy distributions (SEDs) of all known WFs. WFs could be AGB or post-AGB stars with no obvious similarities amongst their SEDs. Further efforts are still needed to improve the identification criteria.link_to_OA_fulltex

Identification of oxygen-rich late/post-asymptotic giant branch stars and water fountains via maser and infrared criteria