By Lindon J.C., Tranter G.E., Holmes J.L. (eds)
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Extra resources for Encyclopedia of Spectroscopy and Spectrometry
Reproduced with permission from Science Photo Library. See Chiroptical Spectroscopy, Oriented Molecules and Anisotropic Systems; Liquid Crystals and Liquid Crystal Solutions Studied by NMR. Reproduced with permission from Science Photo Library. Plate 11 Plate 11 The molecular composition of massive star-forming region in the galaxy. The false color background shows the heart of a massive star-forming region in the constellation of Orion obtained by the Hubble Space Telescope. The red colour is the emission of the molecular hydrogen excited by shocks driven by the powerful wind of a newly formed star in the center of the image.
Indian (1888–1970) physcicist, Nobel Laureate in physics 1930 and discoverer of the Raman effect, a scattering of light by a sample which results in a small fraction of the light being of a different frequency. This phenomenon has applications in analytical chemistry and molecular structure. See Electromagnetic Radiation; Vibrational, Rotational and Raman Spectroscopy, Historical Perspective. Reproduced with permission from Mary Evans Picture Library. 5mM triayl-methyl (TAM) radical. A few representative slices (2424 mm2), obtained from the 3D spatial image are shown.
M. Tielens. Plate 13 Plate 13 Large molecules in the ejecta from a dying star. When solar-type stars grow old they shed much of their mass in the form of a wind much of that in the form of complex molecules. Eventually, the star becomes very hot and sets this ejected material aglow, forming so-called planetary nebulae. The material ejected during this stage will mix with other material present in space and eventually new stars and planetary systems like our own will form these stellar ashes. The false color image shows the emission of molecular hydrogen (red) and atomic hydrogen (white) in the planetary nebula NGC 7027 obtained by the ISO satelite (Infrared Space Observatory).