Results 101 to 110 of about 6,194,227 (235)
Periodic radio and X-ray emission from an accreting white dwarf binary. [PDF]
Rose K +28 more
europepmc +1 more source
Rethinking microtidal systems: Tidal signatures in the fluvial deposits of the Po River, Italy
ABSTRACT In microtidally influenced rivers, tides are generally assumed to leave virtually no signatures in the sedimentary record. However, this hypothesis has been surprisingly poorly tested using modern river analogues, which provide an opportunity to assess whether sedimentary signatures of microtidal regimes can develop in rivers that lack ...
Anna E. van Yperen +6 more
wiley +1 more source
The extended π‐system and low‐lying n‐π∗ transition endow DDOBDiKTa with a synergistic combination of strong spin‐orbit coupling, small reorganization energy and small ΔEST, enabling this blue boron‐nitrogen‐carbonyl hybrid emitter to achieve a fast kRISC of 6.34 × 106 s−1 together with OLEDs showing small efficiency roll‐off, with EQEmax/EQE10000 of ...
Wenrui Wang +6 more
wiley +2 more sources
Jets from a stellar-mass black hole are as relativistic as those from supermassive black holes. [PDF]
Zhang X +17 more
europepmc +1 more source
Nonvolatile nematic order manipulated by strain and magnetic field in a layered antiferromagnet. [PDF]
Feng Z +8 more
europepmc +1 more source
G266.2 1.2 (RX J0852.0 4622) is a member of the emerging class of Galactic supernova remnants (SNRs) which feature X-ray spectra dominated by non-thermal emission.
Stupar, Milorad +5 more
core
Front contact selection governs interfacial stability in CdTe‐based (Cd(Se,Te)) solar cells on ultra‐thin space‐qualified cover glass. Optimized TCO/emitter combinations suppress interdiffusion and deliver up to 16.2% AM0 efficiency with high specific power, demonstrating strong potential for lightweight space photovoltaics.
Aesha P. Patel +17 more
wiley +1 more source
Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262. [PDF]
Kong L +14 more
europepmc +1 more source
High resolution X-ray characterization of mosaic crystals for hard X- and Gamma-ray astronomy
For hard x-ray astronomy in the 70-1000 keV energy range Laue lenses have been proposed where the focusing elements are made of single mosaic crystals, in order to increase the diffraction efficiency with respect to perfect crystals. Suitable crystals to
C Ferrari +3 more
core

