Is X Persei an X-ray Source?

Details Is X Persei an X-ray Source? Is X Persei an X-ray Source?

May 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972natur.237...92c&link_type=abstract

Nature, Volume 237, Issue 5350, pp. 92-93 (1972).

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IT has recently been suggested1,2 that the star X Per (HD 24534) may be associated with the X-ray source 2U 0352 + 30. Other stars identified with X-ray sources are characterized by peculiar spectra with unusual emission lines and by variations in radial velocity which suggests that the sources are binary systems3,4. Because of this we obtained a series of 26 spectra of X Per (including 8 on one night) during the interval December 27, 1971, to March 30, 1972. Dispersions range from 6.5 to 30 Å mm-1, on IIaO, IIaF and IIIaJ emulsions.

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