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- W1966268954 abstract "No X-ray attributable to BETA Persei were detected in the energy range 0.9-10 keV by the MIT X-ray detector on the OSO-7 during an 18-day observation in which numerous radio flares were reported. Upper limits on X-ray emission are established which indicate that the Hjellming model of thermal bremsstrahlung is untenable. (auth)" @default.
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- W1966268954 date "1973-07-01" @default.
- W1966268954 modified "2023-09-27" @default.
- W1966268954 title "Upper Limits to the X-Ray Emission from β Persei during Radio Flares" @default.
- W1966268954 doi "https://doi.org/10.1086/181259" @default.
- W1966268954 hasPublicationYear "1973" @default.
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