On Periodic Variations in the Spectrum of the BOe Star X Persei Associated With the X-Ray Source 3U 0352+30

T.S. Galkina

doi:10.1017/S0074180900037803

On Periodic Variations in the Spectrum of the BOe Star X Persei Associated With the X-Ray Source 3U 0352+30

Published online by Cambridge University Press: 14 August 2015

T.S. Galkina

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T.S. Galkina*: Affiliation:
Crimean Astrophysical Observatory, U.S.S.R.

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The bright BOe star X Persei has been observed for over fifthy years, both as an emission line object and as a variable star.

Type: III. Spectroscopy
Information: Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 189 - 194

DOI: https://doi.org/10.1017/S0074180900037803 [Opens in a new window]

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On Periodic Variations in the Spectrum of the BOe Star X Persei Associated With the X-Ray Source 3U 0352+30

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