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X-ray Emission from Very Dense Stars

Abstract

IN recent years few localized astronomical X-ray sources have been discovered by rocket- and balloon-borne instruments. To explain the X-ray emission by celestial bodies several production mechanisms have been invoked such as the inverse Compton effect, bremsstrahlung in a ‘hot’ plasma cloud, synchrotron radiation and thermal emission.

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SURDIN, M. X-ray Emission from Very Dense Stars. Nature 209, 62–64 (1966). https://doi.org/10.1038/209062b0

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  • DOI: https://doi.org/10.1038/209062b0

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