Results 231 to 240 of about 62,844 (248)

Positive-Type Reversibly Photoswitching Red Fluorescent Protein for Dual-Color Superresolution Imaging with Single Light Exposure for Off-Switching. [PDF]

ACS Nano
Ozaki-Noma R, Wazawa T, Kakizuka T, Shidara H, Takemoto K, Nagai T.   +5 more
europepmc   +1 more source

Crystal structure and Hirshfeld surface analysis of (E)-N-(2-styrylphen-yl)benzene-sulfonamide. [PDF]

Acta Crystallogr E Crystallogr Commun
Albert A M D, Nagaraj A, Somarathinam K, Vinayagam P, Arasambattu K M, Kothandan G.   +5 more
europepmc   +1 more source

Supernovae and supernova remnants [PDF]

, 2001
A supernova explosion is among the most dramatic events that can be seen. The term ‘supernova’ is somewhat misleading, as such an event represents not a new star (that is, a ‘nova’), but instead the end of a star’s life. Nuclear fusion, the energy source of the stars, creates heavier elements from lighter elements.
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Supernovae and Supernova Remnants

1983
Supernovae are the result of explosions which terminate the life of massive stars. The amount of energy released by the supernovae in our galaxy is so large that these explosions provide the dominant energy for the heating of the hot (T ≳ 106 K) IS component and for the kinetic energy of the large scale motions of the interstellar clouds.
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SUPERNOVA EXPLOSIONS AND SUPERNOVA NEUTRINOS

Neutrinos in Physics and Astrophysics, 2000
We summarize the current status of core-collapse supernova theory, in particular as it relates to multi-dimensional effects and neutrino transport . Highlighted are pulsar kicks , neutrino burst signatures, many-body effects, and observed asphericities that may have a bearing on the mechanism of supernova explosions .
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Super Supernovae

Scientific American, 2012
The largest stars die in explosions more powerful than anyone thought possible—some triggered in part by the production of antimatter. ; © 2012 Scientific American, a division of Nature America, Inc. Published online: 15 May 2012.
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