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- W1657154447 abstract "The potential contribution of massive x-ray binaries to the 3–20 key X-ray background has largely been ignored heretofore. It is pointed out that such objects, in the wake of star formation, can contribute at least as much as quasars to the x-ray background, while solving the problems of spectral shape and sky surface density." @default.
- W1657154447 created "2016-06-24" @default.
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- W1657154447 date "1989-01-01" @default.
- W1657154447 modified "2023-09-26" @default.
- W1657154447 title "Star Formation and the X-Ray Background" @default.
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- W1657154447 doi "https://doi.org/10.1007/978-94-009-0919-9_26" @default.
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