Origin of the Hard X-Ray Emission from the Galactic Plane

The Galactic plane is a strong emitter of hard x-rays (2 to 10 kiloelectron volts), and the emission forms a narrow continuous ridge. The currently known hard x-ray sources are far too few to explain the ridge x-ray emission, and the fundamental question of whether the ridge emission is ultimately r...

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Veröffentlicht in:	Science (American Association for the Advancement of Science) 2001-08, Vol.293 (5535), p.1633-1635
Hauptverfasser:	Ebisawa, Ken, Maeda, Yoshitomo, Kaneda, Hidehiro, Yamauchi, Shigeo
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Characteristics and properties of the milky way Climate Data Analysis Earth, ocean, space Energy Exact sciences and technology Field of view Flux density Galactic disks Galactic latitude Galactic planes Galaxies Imaging Milky Way Observation Observations Pixels Point sources Spectra Spiral arms and galactic disk Stars & galaxies Stellar systems. Galactic and extragalactic objects and systems. The universe Unidentified sources and radiation outside the solar system X ray observatories X ray sources X-ray astronomy X-ray sources x-ray bursts X-rays
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