Abstract

SEVERAL investigators have measured the diffuse cosmic X-ray intensity in the 1/4 keV band by means of rocket-borne gas proportional counters1–5. Intensities derived from these measurements have used the assumption that the incident X-rays are continuously distributed in energy over the band-passes of the detectors, and the results disagree. We have therefore reinterpreted existing data, giving consideration to the possibility of line emission (possibly carbon Kα) being superposed on the cosmic X-ray continuum. With this generalization, the discordance of the reported fluxes is substantially reduced. This may be simply an artefact of the existing data, but the possibility that it reflects the existence of a line in the diffuse X-ray background is sufficiently important for us to urge that new data be examined for this possibility as they become available.

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.