Berezinsky V. S., Gaisser, T. K., Halzen, F. & Stanev, T., Diffuse radiation from cosmic ray interactions in the galaxy, Astropart. Phys. 1, pp.281-287, 1993.Berezinsky V. S. et al., Astroparticle Phys. , 1 (199
radiation mechanisms: non-thermalgalaxies: clusters: generalgalaxies: clusters: individual: A 521galaxies: clusters: individual: A 697galaxies: clusters: individual: A1682In this paper we present new high sensitivity 153 MHz Giant Meterwave Radio Telescope follow-up observations of the diffuse steep ...
radiation名— 辐射名 · 放射名 · 輻射名 · 放射线名 · 幅射名 铺散动 ▾ 外部资源(未审查的) In pursuance with the objective of the Organization to maintain, increaseanddiffuseknowledge, UNESCO affirms that all its publications (e.g. ...
radiofrequency cosmic radiationThe GalaxyX-ray astronomy/ A9850 The Galaxy, extragalactic objects and systemsMEASUREMENTS of the low-resolution, low-frequency, radio spectra in the direction of the galactic poles show a significant difference between the two hemispheres. Spectra for the north and ...
Galaxy: Diffuse RadiationGamma-Ray Background: ExtragalacticThe Energetic Gamma-Ray Experiment Telescope (EGRET) on the Compton Observatory has surveyed the sky for high energy gamma-ray emission and has observed emission from several different source classes including active galaxies, pulsars, solar ...
local galaxyradiationsscatteringx radiation interstellar material/x-ray scattering by, background, (tcosmic x-ray sources/distribution in milky way, (tCooke, Griffiths and Pounds 1 have recently reported an excess in the diffuse X-ray background intensity observed at low galactic latitudes, ...
Diffuse Radio Emission in Abell 754 来自 Semantic Scholar 喜欢 0 阅读量: 41 作者: R Kale,KS Dwarakanath 摘要: We present a low frequency study of the diffuse radio emission in the galaxy cluster A754. We present new 150 MHz image of the galaxy cluster A754 made with the Giant Metrewave...
We present an analysis of the diffuse ultraviolet (UV) background in a low latitude region near the Aquila Rift based on observations made by the Galaxy Evolution Explorer (GALEX). The UV background is at a level of about 2000 ph cm^-2 s^-1 sr^-1 \AA^-1
The cooling time is often much shorter than 1 Gyr, therefore some source of heating is necessary to balance the radiation losses. At present, it is widely accepted that the source of heating in cool-core clusters is the AGN activity of the brightest cluster galaxy at the center (see ...
Free Essays from Bartleby | Kelly Quach Instructor Eliza Ebro English 101: Section 93 11 October 2017 The Aesthetic and Science Behind Sunsets Jo Walton once...