Abstract
VARIOUS populations1–3 of ad hoc stellar objects have been proposed to explain the soft X-ray background, in particular the component observed from the galactic plane.
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CAVALLO, G., HORSTMAN, H. Soft X-ray Background and Flare Stars. Nature Physical Science 235, 110 (1972). https://doi.org/10.1038/physci235110a0
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DOI: https://doi.org/10.1038/physci235110a0
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