X-ray background
id:
x-ray-background-316-5827597
title:
X-ray background
text:
The observed X-ray background is thought to result from, at the "soft" end, galactic X-ray emission, the "galactic" X-ray background, and, at the "hard" end, from a combination of many unresolved X-ray sources outside of the Milky Way, the "cosmic" X-ray background (CXB). The galactic X-ray background is produced largely by emission from hot gas in the Local Bubble within 100 parsecs of the Sun. Deep surveys with X-ray telescopes, such as the Chandra X-ray Observatory, have demonstrated that aro
brand slug:
wiki
category slug:
encyclopedia
description:
original url:
https://en.wikipedia.org/wiki/X-ray_background
date created:
date modified:
2019-12-27T06:25:31Z
main entity:
{"identifier":"Q1345176","url":"https://www.wikidata.org/entity/Q1345176"}
image:
fields total:
13
integrity:
13