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相关论文: Spiral Galaxies - classical description of spiral …

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We describe how a simple class of out of equilibrium, rotating and asymmetrical mass distributions evolve under their self-gravity to produce a quasi-planar spiral structure surrounding a virialized core, qualitatively resembling a spiral…

星系天体物理 · 物理学 2017-12-08 David Benhaiem , Michael Joyce , Francesco Sylos Labini

Using an equation of motion for a self-gravitating filament, we show how galactic spiral arms might be created and sustained. We find that the combination of differential rotation of the galactic disk and the self-gravity of the arm (as…

星系天体物理 · 物理学 2013-03-04 Gregory Buck

Most fully developed galaxies have a vivid spiral structure, but the formation and evolution of the spiral structure are still an enigma in astrophysics. In this paper, according to the standard Newtonian gravitational theory and some…

综合物理 · 物理学 2009-05-16 Ying-Qiu Gu

Spiral density wave theory attempts to describe the spiral pattern in spiral galaxies in terms of a long-lived wave structure with a constant pattern speed in order to avoid the winding dilemma. The pattern is consequently a rigidly…

星系天体物理 · 物理学 2015-06-03 Robert J. J. Grand , Daisuke Kawata , Mark Cropper

It is well established that many galaxies, like our Milky Way, exhibit spiral patterns. The entire galactic disc rotates about the galactic centre with different speeds; higher closer to the centre, lower at greater distances - that is,…

高能物理 - 唯象学 · 物理学 2016-02-16 A. Rustamov , J. N. Rustamov

The most important theory of the spiral arms of galaxies is the density wave theory based on the Lin-Shu dispersion relation. However, the density waves move with the group velocity towards the inner Lindblad resonance and tend to…

星系天体物理 · 物理学 2022-10-26 George Contopoulos

The measured rotation velocity profiles of mature spiral galaxies are successfully described with a gravitational model consisting of a thin axisymmetric disk of finte radius. The disk is assumed uniformly thin but with variable radial mass…

天体物理学 · 物理学 2008-03-06 James Q. Feng , C. F. Gallo

Observations reveal that mature spiral galaxies consist of stars, gases and plasma approximately distributed in a thin disk of circular shape, usually with a central bulge. The rotation velocities quickly increase from the galactic center…

天体物理学 · 物理学 2008-04-22 C. F. Gallo , James Q. Feng

Spiral arms are the defining features of broad morphological classes of disc galaxies, but their nature and influence on galaxy evolution is still under debate. A key diagnostic for their nature is the spiral arm pattern speed: the radial…

天体物理仪器与方法 · 物理学 2025-12-22 Robert J. J. Grand , Martin Roth

Spiral density wave theory attempts to describe the spiral pattern in spiral galaxies in terms of a long-lived wave structure with a constant pattern speed in order to avoid the winding dilemma. The pattern is consequently a rigidly…

星系天体物理 · 物理学 2015-05-30 Daisuke Kawata , Robert J. J. Grand , Mark Cropper

We present a map of the spiral structure of the Galaxy, as traced by molecular CS emission associated with IRAS sources which are believed to be compact HII regions. The CS line velocities are used to determine the kinematic distances of…

星系天体物理 · 物理学 2015-05-20 J. R. D. Lepine , A. Roman-Lopes , Zulema Abraham , T. C. Junqueira , Yu. N. Mishurov

Galactic rotation curve is a powerful indicator of the state of the gravitational field within a galaxy. The flatness of these curves indicates the presence of dark matter in galaxies and their clusters. In this paper, we focus on the…

广义相对论与量子宇宙学 · 物理学 2023-11-28 Gayatri Mohan , Umananda Dev Goswami

It is discussed that the formation of the spiral galaxies is driven by the cosmic background rotation, not a result of an isolated evolution proposed by the density wave theory. To analyze the motions of the galaxies, a simple double…

星系天体物理 · 物理学 2018-02-20 Zexin Cao , Ling Liu , Tingting Zheng

The spiral galaxies, including our galaxy, are created by the gravito-radiative forces generated by colliding black holes at the center of quasars. The gravito-radiative force is predicted by Einstein's general relativity. A quasar is…

综合物理 · 物理学 2008-02-01 Masataka Mizushima

We discuss a model for the Milky Way obtained by fitting the observed terminal velocities with the radial acceleration relation. The resulting stellar surface density profile departs from a smooth exponential disk, having bumps and wiggles…

星系天体物理 · 物理学 2019-11-06 Stacy McGaugh

In an equilibrium axisymmetric galactic disc, the mean galactocentric radial and vertical velocities are expected to be zero everywhere. In recent years, various large spectroscopic surveys have however shown that stars of the Milky Way…

星系天体物理 · 物理学 2015-06-19 Carole Faure , Arnaud Siebert , Benoit Famaey

One of the scenarios for the formation of grand-design spiral arms in disky galaxies involves their interactions with a satellite or another galaxy. Here we consider another possibility, where the perturbation is instead due to the…

星系天体物理 · 物理学 2016-12-28 Marcin Semczuk , Ewa L. Lokas , Andres del Pino

We investigate the possibility of describing the spiral pattern of the Milky Way in terms of a model of superposition 2- and 4-armed wave harmonics (the simplest description, besides pure modes). Two complementary methods are used: a study…

天体物理学 · 物理学 2009-10-31 J. R. D. Lepine , Yu. N. Mishurov , S. Yu. Dedikov

We propose a new, more realistic, description of the perturbed gravitational potential of spiral galaxies, with spiral arms having Gaussian-shaped groove profiles. We investigate the stable stellar orbits in galactic disks, using the new…

星系天体物理 · 物理学 2015-06-12 T. C. Junqueira , J. R. D. Lépine , C. A. S. Braga , D. A. Barros

We propose a new theory to explain the formation of spiral arms and of all types of outer rings in barred galaxies. We have extended and applied the technique used in celestial mechanics to compute transfer orbits. Thus, our theory is based…

天体物理学 · 物理学 2007-12-31 M. Romero-Gomez , E. Athanassoula , J. J. Masdemont , C. Garcia-Gomez
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