Abstract
IN many respects the most recent nova is following the usual course in its spectral changes. The present spectrum is a medley of bright bands and of absorption lines: the bright hydrogen bands are accompanied by a number of absorption components on the side of shorter wave-length, while corresponding to each component and with the same Doppler displacement are a number of absorption lines due to atoms of Fe+, Ti+, Cr+, Ca+, etc.
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Bowen, Astrophys. J., 81, 12; 1935.
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BEER, A., STRATTON, F. Spectrum of Nova Herculis, 1934. Nature 135, 346 (1935). https://doi.org/10.1038/135346a0
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DOI: https://doi.org/10.1038/135346a0
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