4.7 Article

Spectrum of hot water in the 4750-13 000 cm-1 wavenumber range (0.769-2.1 μm)

Journal

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 387, Issue 3, Pages 1093-1098

Publisher

WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2008.13234.x

Keywords

line : identification; molecular data; sunspots; infrared : stars

Funding

  1. EPSRC [EP/E043674/1] Funding Source: UKRI

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The high resolution laboratory spectrum of hot water vapour has been recorded in the 500-13 000 cm(-1) wavenumber range and we report on the analysis of the 4750-13 000 cm(-1) (0.769-2.1 mu m) portion. The emission spectrum was recorded using an oxy-acetylene welding torch and a Fourier transform spectrometer. Line assignments in the laboratory spectrum as well as in an absorption spectrum of a sunspot umbra were made with the help of the BT2 line-list. Our torch spectrum is the first laboratory observation of the 9300 angstrom 'steam bands' seen in M-stars and brown dwarfs.

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