Results 181 to 190 of about 3,393,330 (216)
Hebbian instruction of axonal connectivity by endogenous correlated spontaneous activity. [PDF]
Matsumoto N +3 more
europepmc +1 more source
Stellar feedback drives the baryon deficiency in low-mass galaxies. [PDF]
Yu H +10 more
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Tunable photofluorochromic switch driven by dynamic through-space conjugation. [PDF]
Xiong Z +9 more
europepmc +1 more source
The role of native defects in organic-inorganic hybrid zinc halide luminescent materials. [PDF]
Zhang Y, Liu Q, Wang R, Li X, Liu X.
europepmc +1 more source
Direct Samples of Interstellar and Interplanetary Material with IMAP. [PDF]
Szalay JR +21 more
europepmc +1 more source
Supernova Remnants Dynamics [PDF]
AbstractSupernova remnants are the site of a number of physical processes (shock-heating, non-equilibrium ionization, hydrodynamic instabilities, particle acceleration, magnetic field amplification). Their related emission processes provide us with a large set of observational data.
Anne Decourchelle
exaly +3 more sources
Dynamics of Supernova Bounce in Laboratory [PDF]
We draw attention to recent high explosive (HE) experiments which provide compression of macroscopic amount of matter to high, even record, values of pressure in comparison with other HE experiments. The observed bounce after the compression corresponds to processes in core-collapse supernova explosions after neutrino trapping.
Andrey Yudin +2 more
exaly +4 more sources
ALMA Spectral Survey of Supernova 1987A – Molecular Inventory, Chemistry, Dynamics and Explosive Nucleosynthesis [PDF]
We report the first molecular line survey of Supernova 1987A in the millimetre wavelength range. In the Atacama Large Millimeter/submillimeter Array (ALMA) 210–300 and 340–360 GHz spectra, we detected cold (20–170 K) CO, 28SiO, HCO+ and SO, with weaker ...
Serena Viti +2 more
exaly +2 more sources
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Nuclear Quests for Supernova Dynamics and Nucleosynthesis
Progress in Particle and Nuclear Physics, 2011Nuclear physics plays a crucial role in various aspects of core-collapse supernovae. The collapse dynamics is strongly influenced by electron captures. Using the modern many-body theory, improved capture rates have been derived recently with the important result that the process is dominated by capture on nuclei until neutrino trapping is achieved ...
Gabriel Martínez-Pinedo, K Langanke
exaly +3 more sources
Supernovae and interstellar gas dynamics
Symposium - International Astronomical Union, 1967The efficiency of the transfer of energy from supernovae into interstellar cloud motions is investigated. A lower limit of about 0·002 is obtained, but values near 0·01 are more likely. Taking all uncertainties in the theory and observations into account, the energy per supernova, in the form of relativistic particles or high-velocity matter, needed to
F. D. Kahn, L. Woltjer
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