Results 191 to 200 of about 2,169 (225)

Proton Acceleration with Relativistic Electromagnetic Shock. [PDF]

Adv Sci (Weinh)
Xiao T, Zhang X, Kong F, Zheng X, Gong Z, Shen B.   +5 more
europepmc   +1 more source

"Ammonia Induced Framework Transformations and Spin-Crossover in Fe(II) Hofmann MOFs". [PDF]

Inorg Chem
Pacheco M, Jesuman A, Maqueda-Márquez H, González-Platas J, Gaspar AB.   +4 more
europepmc   +1 more source

Chromosome scale genomes of two invasive Adelges species enable virtual screening for selective adelgicides. [PDF]

G3 (Bethesda)
Glendening AM, Stephens C, Vuruputoor VS, Chaganti T, Myles MN, Stern DL, Abdelalim M, Juang YP, Hogenhout SA, Mathers TC, Pauloski N, Cernak TA, Wegrzyn JL, Fetter KC.   +13 more
europepmc   +1 more source

Transport of Electrons in Tangled Magnetic Fields. [PDF]

Space Sci Rev
Verscharen D, Jeffrey N, Artemyev A, Coburn JT, Kunz MW, Pezzi O, Riquelme M, Svenningsson I, Wilson Iii LB.   +8 more
europepmc   +1 more source

A reference-grade genome assembly data of sika deer in Hokkaido, Japan, <i>Cervus nippon yesoensis</i>. [PDF]

Data Brief
Matsumoto Y, Nagata J, Matsuura Y, Iijima H.   +3 more
europepmc   +1 more source

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Nuclear quests for supernova dynamics and nucleosynthesis

Progress in Particle and Nuclear Physics, 2011
Nuclear 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 ...
G Martínez-Pinedo
exaly   +3 more sources

ALMA spectral survey of Supernova 1987A – molecular inventory, chemistry, dynamics and explosive nucleosynthesis [PDF]

Monthly Notices of the Royal Astronomical Society, 2017
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 ...
M Matsuura, Remy Indebetouw, S Woosley   +2 more
exaly   +2 more sources

Supernovae and interstellar gas dynamics

Symposium - International Astronomical Union, 1967
The 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
openaire   +1 more source