Abstract
THE observations of the new star in Perseus have not decreased in interest since they were last referred to in NATURE. Strictly according to precedent a nebular spectrum, somewhat similar to that observed by Gothard in Nova Aurigæ, followed the disappearance of the dark lines in the spectrum; but about the same time a new phenomenon in relation to Nova was observed; the star behaved like a “collision-variable.”
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Nova Persei . Nature 63, 540–541 (1901). https://doi.org/10.1038/063540b0
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DOI: https://doi.org/10.1038/063540b0