Optical Circular Polarization of X Persei
THE possible identification 1 of X Per with the X-ray source 2 2ASE 0352+ 30 has stimulated interest in other properties of the star. In addition to detailed observations of the optical spectrum by Crampton and Hutchings 3 , attempts to observe radio emissions 4 of the object at 21 cm have yielded n...
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| Veröffentlicht in: | Nature (London) Phys. Sci. 241: No. 105, 5(1 Jan 1973) 5(1 Jan 1973), 1973-01, Vol.241 (105), p.5-5 |
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| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | eng |
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| Online-Zugang: | Volltext |
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| Zusammenfassung: | THE possible identification
1
of X Per with the X-ray source
2
2ASE 0352+ 30 has stimulated interest in other properties of the star. In addition to detailed observations of the optical spectrum by Crampton and Hutchings
3
, attempts to observe radio emissions
4
of the object at 21 cm have yielded no positive results. An attempt by Baud and Tinbergen
5
to observe circular polarization in visible light showed no component greater than 0.02 of the total intensity. |
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| ISSN: | 0300-8746 2058-1106 |
| DOI: | 10.1038/physci241005a0 |