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Cited article:

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Water content and wind acceleration in the envelope around the oxygen-rich AGB star IK Tauri as seen byHerschel/HIFI

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A HIFI preview of warm molecular gas aroundχCygni: first detection of H2O emission toward an S-type AGB star

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THE MASS-LOSS RETURN FROM EVOLVED STARS TO THE LARGE MAGELLANIC CLOUD. II. DUST PROPERTIES FOR OXYGEN-RICH ASYMPTOTIC GIANT BRANCH STARS

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Probing the mass-loss history of AGB and red supergiant stars from CO rotational line profiles

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The ISO Long Wavelength Spectrometer line spectrum of VY Canis Majoris and other oxygen-rich evolved stars

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Polarisation observations of VY Canis Majoris H2O 532–441620.701 GHz maser emission with HIFI

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RED SUPERGIANTS AS POTENTIAL TYPE IIn SUPERNOVA PROGENITORS: SPATIALLY RESOLVED 4.6 μm CO EMISSION AROUND VY CMa AND BETELGEUSE

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A Search for Temperature and Density Variations in NGC 7027 with theHubble Space Telescope

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Probing the mass-loss history of the unusual Mira variable R Hydrae through its infrared CO wind

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Detection of “parent” molecules from the inner wind of AGB stars as tracers of non-equilibrium chemistry

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Towards a spectral technique for determining material geometry around evolved stars: application to HD 179821

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The variable mass loss of the AGB star WX Piscium as traced by the CO J = 1-0 through 7-6 lines and the dust emission

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The Molecular Envelope around the Red Supergiant VY CMa

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