Results 111 to 120 of about 526 (138)
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Proceedings of the International Astronomical Union, 2019
AbstractThe venerable problem of what causes the spiral features in disk galaxies is nearing a solution. In previous work, we have shown that transient spirals in simulations result from the superposition of a few coherent waves that have many properties of modes.
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AbstractThe venerable problem of what causes the spiral features in disk galaxies is nearing a solution. In previous work, we have shown that transient spirals in simulations result from the superposition of a few coherent waves that have many properties of modes.
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Dark matter in spiral galaxies
Philosophical Transactions of the Royal Society of London. Series A, Mathematical and Physical Sciences, 1986Abstract Mass models of spiral galaxies based on the observed light distribution, assuming constant M /L for bulge and disc, are able to reproduce the observed rotation curves in the inner regions, but fail to do so increasingly towards and beyond the edge of the visible material.
VANALBADA, TS, SANCISI, R
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Nature, 1988
The concept of the turbulent dynamo in interstellar gas combined with the discovery of global magnetic structures in spiral galaxies has led to a consistent picture of galactic magnetism. Large-scale magnetic fields are generated and maintained by helical turbulent motions of interstellar gas and by differential galactic rotation.
Alexander Ruzmaikin +2 more
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The concept of the turbulent dynamo in interstellar gas combined with the discovery of global magnetic structures in spiral galaxies has led to a consistent picture of galactic magnetism. Large-scale magnetic fields are generated and maintained by helical turbulent motions of interstellar gas and by differential galactic rotation.
Alexander Ruzmaikin +2 more
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Comparison of the Galaxy with External Spiral Galaxies
1987In this chapter some areas of comparative exploration in our and external galaxies are reviewed and discussed. Photometric parameters for the Galaxy are derived. The radial scalelength is 5.0 ± 0.5 kpc, and this makes our Galaxy (and M31) unusually large unless Ho = 65 ± 10 km s−1 Mpc−1. Surface photometry of external edge-on galaxies, in particular of
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Vortices degradation and periodical variation in spiral micromixers with various spiral structures
International Journal of Heat and Mass Transfer, 2022Yukui Cai, Bing Wang, Yi Wan
exaly
Spiral wound modules and spacers
Journal of Membrane Science, 2004D F Fletcher, A G Fane, P R Neal
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Vertically Conductive MoS2 Spiral Pyramid
Advanced Materials, 2016Young Hee Lee, Thuc Hue Ly, Jiong Zhao
exaly
Spiral wave chimera in two-dimensional nonlocally coupled Fitzhugh–Nagumo systems
Chaos, Solitons and Fractals, 2018Qionglin Dai +2 more
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