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Bisymmetric Spiral Magnetic Fields in Spiral Galaxies

1987
A radio polarization analysis was presented in 1978 by TOSA and FUJIMOTO [1] to determine a large-scale configuration of magnetic fields in the spiral galaxy M51. On the basis of the distributions of planes of polarization at 6 cm and 21 cm [2], they determined the rotation measures (RMs) of the Faraday effect and the intrinsic polarization angles. The
openaire   +1 more source

Phenomenology of Spiral Galaxies

1975
Galaxies have probably been formed from fluctuations in density and motion in the universe. Many cosmologists have suggested that the separation into individual units took place around the time of decoupling of matter and radiation, when the radius of the universe was about 1/1000th of the present radius.
openaire   +1 more source

Spiral Metalens for Phase Contrast Imaging

Advanced Functional Materials, 2022
Gun-Yeal Lee   +2 more
exaly  

Spiral density waves in a young protoplanetary disk

Science, 2016
Laura M Perez   +2 more
exaly  

Tri‐Spiral Donor for High Efficiency and Versatile Blue Thermally Activated Delayed Fluorescence Materials

Angewandte Chemie - International Edition, 2019
Xinyi Cai, Dongcheng Chen, Shi-Jian Su
exaly  

Quantum digital spiral imaging

Light: Science and Applications, 2014
Lixiang Chen, Jacquiline Romero
exaly  

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