Herschel SPIRE and PACS observations of the red supergiant VY CMa: analysis of the molecular line spectra

@article{Matsuura2013HerschelSA,
  title={Herschel SPIRE and PACS observations of the red supergiant VY CMa: analysis of the molecular line spectra},
  author={M. Matsuura and J. Yates and M. Barlow and B. Swinyard and P. Royer and J. Cernicharo and L. Decin and R. Wesson and E. Polehampton and J. Blommaert and M. Groenewegen and G. V. Steene and P. J. U. C. London and UK. and R. Laboratory and K. Leuven and Belgium and INTA-CSIC and Spain. and E. Observatory and Chile University of Lethbridge and Canada. and R. O. O. Belgium},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={437},
  pages={532-546}
}
We present an analysis of the far-infrared and submillimetre molecular emission-line spectrum of the luminous M-supergiant VY CMa, observed with the Spectral and Photometric Imaging Receiver (SPIRE) and Photodetector Array Camera and Spectrometer for Herschel spectrometers aboard the Herschel Space Observatory. Over 260 emission lines were detected in the 190–650 μm SPIRE Fourier Transform Spectrometer spectra, with one-third of the observed lines being attributable to H2O. Other detected… Expand
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