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Radio Spectrum of H Atom n=110—>109n=139—>137 He C | |
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CECILIA PAYNE-GAPOSCHKIN: ASTRONOMER AND ASTROPHYSICIST 1900-1980 "THE MOST BRILLIANT Ph.D. THESIS EVER WRITTEN IN ASTRONOMY"
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CO J=1—0 in Orion 115.3GHz
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Horsehead nebula in Orion. Observed by microwave emission of carbon monoxide The green and yellow regions are of greater concentrations of carbon monoxide. Cal Tech
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93.206GHz 108.724
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FluxFlux GHz Ap. J.472, L49 (1996)
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Ionization Potential H = 109678.758 cm -1 E = -IP/n 2 ∆E = -IP((1/(n 2 ))-(1/(n+1) 2 ))
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