... Emission from these cosmicrays explains the WMAP Haze observed at microwave wavelengths around the Galactic centre as well as ... These giant shocks may also be the dominant source of cosmicrays in the Galaxy-as-a-whole above energies of ~10^15 eV.. ...
... ionization profile, with contributions from Xrays, cosmicrays and radioactive decay ... object are non-thermal: Interstellar cosmicrays, emitted by the magnetically active ...
... SNe Ia) are also the dominant contributor to iron-group nucleosynthesis and leading candidates for the elusive sites of high energy cosmicrays, the p-process isotopes, and the positrons responsible for the 511 keV annihilation signal in our Galaxy ...
... Study of the radio emission from the Interstellar Medium (related to cosmicrays). ... Pulsars, Supernovae or Hypernovae · Supernovae, heat the ISM and create cosmicrays ... Most cosmicrays may be the result of supernovae blast waves. ...
... measurements of cosmic star-formation, intergalactic magnetic fields, the cosmic non-thermal energy density, sources of neutrinos and cosmicrays, and provide constraints on dark matter and several extensions of the standard model of particle physics ...
... The method [2] incorporates a realistic ionization profile, produced by cosmicrays, Xrays and radioactive decay. ... field for the minimum-solar nebula disk and including the ionization provided by cosmicrays, X-rays and radioactive decay ...
... X-ray Observations of Pictor A: High Energy CosmicRays in a Radio Galaxy A. S ... A) galaxies: jets galaxies: nuclei ISM: cosmicrays X-rays: galaxies 1 ... common assumption of equipartition of energy between cosmicrays and magnetic fields ...
... spuriously high pixels, due to cosmicrays (actually often terrestrial background ... available which try to get rid of cosmicrays by filtering out any really sharp ...
... was also used to automatically locate cosmicrays and stars in the galaxy images ... Stars and cosmicrays were distinguished using the DAOPHOT sharpness ... The cosmicrays were removed by replacing aected pixels with the biweight of ...
... But Hubble cannot expose for more than ~ 20-40 minutes at a time without the signal being buried in cosmicrays. ... Such as confusion noise, scattered light, flat fielding errors, weak cosmicrays, unstable biases etc. ...