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Note on the New Star in Perseus

Published online by Cambridge University Press:  15 September 2014

The Astronomer-Royal for Scotland
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Extract

We are again indebted to Dr T. D. Anderson of this city for the announcement of the discovery of a new star, which was first seen by him at 2h 40m a.m., G.M.T., on Friday, the 22nd February.

Type
Proceedings
Information
Proceedings of the Royal Society of Edinburgh , Volume 23 , 1902 , pp. 365 - 369
Copyright
Copyright © Royal Society of Edinburgh 1902

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References

note * page 366 Note added March 15.—While the band at 486 μμ is undoubtedly due to hydrogen, which is also present in the spectrum of the nebulæ, that at 501 μμ does not appear, as later measurements showed, to coincide with the chief nebula line at 500·7, but is probably identical with the chromospheric line 501·8 due to iron.