Results 111 to 120 of about 37,813 (241)
X-rays from supernova remnants [PDF]
13 pages, 18 figures. To appear in the Proceedings of the 270. WE-Heraeus Seminar on Neutron Stars, Pulsars and Supernova Remnants, Jan. 21-25, 2002, Physikzentrum Bad Honnef, eds W. Becker, H. Lesch & J. Truemper.
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Observations at 408 MHz of Supernova Remnants in the LMC [PDF]
J. N. Clarke
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Gamma-rays and neutrinos from very young supernova remnants [PDF]
R.J. Protheroe, W. Bednarek, Q. Luo
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Proper motions of Hα filaments in the supernova remnant RCW 86 [PDF]
E. A. Helder +6 more
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Supernova Ejecta with Crystalline Silicate Dust in the Supernova Remnant MSH 15–52
IRAS 15099-5856 in the young supernova remnant (SNR) MSH 15−52 is the first and only SNR-associated object with crystalline silicate dust detected so far, although its nature and the origin of the crystalline silicate are still unclear. In this paper, we
Hyun-Jeong Kim +2 more
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Supernova 1604, Kepler’s Supernova, and Its Remnant [PDF]
Supernova 1604 is the last Galactic supernova for which historical records exist. Johannes Kepler's name is attached to it, as he published a detailed account of the observations made by himself and European colleagues. Supernova 1604 was very likely a Type Ia supernova, which exploded 350 pc to 750 pc above the Galactic plane.
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Distances to Recent Near-Earth Supernovae from Geological and Lunar 60Fe
Near-Earth supernova blasts which engulf the solar system have left traces of their ejecta in the geological and lunar records. There is now a wealth of data on live radioactive ^60 Fe pointing to a supernova at 3 Myr ago, as well as the recent discovery
Adrienne F. Ertel, Brian D. Fields
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Spitzer Observations of Supernova Remnant IC 443 [PDF]
A. Noriega‐Crespo +6 more
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Light Curve Models of Supernovae and X-ray spectra of Supernova Remnants [PDF]
С. И. Блинников +3 more
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Evidence of Gradients of Density and Magnetic Field in the Remnant of Tycho’s Supernova
By using surface brightness maps of Tycho’s supernova remnant (SNR) in radio and X-rays, along with the properties of thermal and synchrotron emission, we have derived the postshock density and magnetic field (MF) strength distributions over the ...
Oleh Petruk +7 more
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