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The Herschel SPIRE Fourier Transform Spectrometer Spectral Feature Finder – III. Line identification and off-axis spectra

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Late stages of stellar evolution – Herschel’s contributions

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The complex dust formation zone of the AGB star IRC+10216 probed with CARMA 0.25 arcsec angular resolution molecular observations

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MESS (Mass-loss of Evolved StarS), aHerschelkey program

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A spectroscopic case for SPSi detection: The third-row in a single molecule

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The role of ultraviolet photons in circumstellar astrochemistry

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Discovery of multiple dust shells beyond 1 arcmin in the circumstellar envelope of IRC +10216 usingHerschel/PACS

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Water in IRC+10216: a genuine formation process by shock-induced chemistry in the inner wind

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DISCOVERY OF TIME VARIATION OF THE INTENSITY OF MOLECULAR LINES IN IRC+10216 IN THE SUBMILLIMETER AND FAR-INFRARED DOMAINS

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The inner wind of IRC+10216 revisited: new exotic chemistry and diagnostic for dust condensation in carbon stars

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The Abundance of C2H4in the Circumstellar Envelope of IRC+10216

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Molecular abundances in the inner layers of IRC +10216

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The abundance of28Si32S,29Si32S,28Si34S, and30Si32S in the inner layers of the envelope of IRC+10216

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Detection of anhydrous hydrochloric acid, HCl, in IRC +10216 with the HerschelSPIRE and PACS spectrometers

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A high-resolution line survey of IRC +10216 withHerschel/HIFI

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Theoretical Studies of SiC4H2 Isomers Delineate Three Low-Lying Silylidenes Are Missing in the Laboratory

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Study of CS, SiO, and SiS abundances in carbon star envelopes: assessing their role as gas-phase precursors of dust

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Warm water vapour in the sooty outflow from a luminous carbon star

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DOI: 10.1038/nature09344
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