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Bisymmetric Spiral Magnetic Fields in Spiral Galaxies
1987A 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
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Phenomenology of Spiral Galaxies
1975Galaxies 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.
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Spiral morphology in an intensely star-forming disk galaxy more than 12 billion years ago
Science, 2021Takafumi Tsukui, Satoru Iguchi
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A repeating fast radio burst source localized to a nearby spiral galaxy
Nature, 2020Benito Marcote +2 more
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The Identification of a Dusty Multiarm Spiral Galaxy at z = 3.06 with JWST and ALMA
Astrophysical Journal Letters, 2023Yunjing Wu, Zheng Cai, Fengwu Sun
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The Galaxy in Context: Structural, Kinematic, and Integrated Properties
Annual Review of Astronomy and Astrophysics, 2016Joss Bland-Hawthorn, Ortwin Gerhard
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High velocity dispersion in a rare grand-design spiral galaxy at redshift z = 2.18
Nature, 2012Alice E Shapley +2 more
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