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Atombau und Spektrallinien. 1.
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Atombau und Spektrallinien. 2.
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Atomic energy levels as derived from the analyses of optical spectra. 1. the spectra of hydrogen ... /
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Atomic energy levels as derived from the analyses of optical spectra. volume 0002 : The spectra of chromium, manganese, iron, cobalt, nickel, copper, zinc, gallium, germanium, arsenic, selenium, bromine, krypton, rubidium, strontium, yttrium, zirconium, and niobium.
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Atomic energy levels - the rare earth elements : The spectra of lanthanum, cerium, praseodymium, neodymium, promethium, samarium, europium, gadolinium, terbium, dysprosium, holmium, erbium, thulium, ytterbium, and lutetium.
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Atomic energy levels vol 0003: the spectra of molybdenum, technetium, ruthenium, rhodium, palladium, silver, cadmium, indium, tin, antimony, tellurium, iodine, xenon, cesium, barium, lanthanum, hafnium, tantalum, tungsten, rhenium, osmium, iridium, platinum, gold, mercury, thallium, lead, bismuth, polonium, radon, radium, and actinium.
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Atomic spectra and radiative transitions.
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Atomic spectra in the vacuum ultraviolet from 2250 to 1100 A. pt 0001 : Al, C, Cu, Fe, Ge, Hg, Si (H2)
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Junkes, J.
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Atomic transition probabilities of carbon, nitrogen, and oxygen : a critical data compilation /
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Atomic transition probabilities: scandium through manganese.
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Atomic transition probabilities vol 0001: hydrogen through neon, a critical data compilation /
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Excitation of atoms and broadening of spectral lines : 38 tables /
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Hydrogen I - phosphorus XV.
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Hydrogen I - phosphorus XV.
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Manganese I - XXV.
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Sulfur I - titanium XXII.
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The theory of atomic spectra /
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Vanadium I - chromium XXIV.
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Wavelength tables with intensities in arc, spark, or discharge tube of more than 100,000 spectrum lines, most strongly emitted by the atomic elements under normal conditions of excitation, between 10,000 A and 2000 A, arranged in order of decreasing wavelengths /
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Wavelengths and transition probabilities for atoms and atomic ions. 1, 2. wavelenghts transition probabilities.
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