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On the chemistry and distribution of HOC+ in M82: More evidence for extensive PDRs
A. Fuente, S. Garcia-Burillo, A. Usero +8
The molecular gas composition in the inner 1 kpc disk of the starburst galaxy M82 resembles that of Galactic Photon Dominated Regions (PDRs). In particular, large abundances of the…
Water in the Near IR spectrum of Comet 8P/Tuttle
R. J. Barber, S. Miller, N. Dello Russo +3
High resolution spectra of Comet 8P/Tuttle were obtained in the frequency range 3440.6-3462.6 cm-1 on 3 January 2008 UT using CGS4 with echelle grating on UKIRT. In addition to rec…
A H13CN/HN13C linelist, model atmospheres and synthetic spectra for carbon stars
G. J. Harris, F. C. Larner, J. Tennyson +3
A line list of vibration-rotation transitions for 13C substituted HCN is presented. The line list is constructed using known experimental levels where available, calculated levels…
A potential new method for determining the temperature of cool stars
S. Viti, H. R. A. Jones, M. J. Richter +3
We present high resolution (R = 90,000) mid-infrared spectra of M dwarfs. The mid infrared region of the spectra of cool low mass stars contain pure rotational water vapour transit…
Spectral analysis of high resolution near-infrared spectra of ultra cool dwarfs
Yu. Lyubchik, H. R. A. Jones, Ya. V. Pavlenko +5
We present an analysis of high resolution spectra in the J band of five ultra cool dwarfs from M6 to L0. A new ab initio water vapour line list and existing line lists of FeH and C…
Water vapour in the atmosphere of a transiting extrasolar planet
Giovanna Tinetti, Alfred Vidal-Madjar, Mao-Chang Liang +10
Water is predicted to be among, if not the most abundant molecular species after hydrogen in the atmospheres of close-in extrasolar giant planets (hot-Jupiters) Several attempts ha…