Kinematics and dynamics of the Galactic disc
Martin Lopez-Corredoira

TL;DR
This paper reviews various hypotheses explaining the Milky Way disc's complex features and kinematic anomalies, emphasizing the role of intergalactic matter accretion and gravitational interactions in shaping the galaxy's structure.
Contribution
It provides a comprehensive review of the potential causes of Galactic disc anomalies, highlighting the significance of intergalactic matter accretion and gravitational effects.
Findings
Galactic features are sensitive to internal and external forces.
Accretion of intergalactic matter explains many observed anomalies.
Other hypotheses only partially account for the observations.
Abstract
The Milky Way disc presents a warp, a flare, lopsidedness and other deviations from a purely axisymmetrical double exponential density component, both for the stellar and the gas component. Moreover, recent large-scale extended kinematics maps of Gaia data have shown significant departures from circularity in the mean orbits with radial Galactocentric velocities between -20 and +20 km/s and vertical velocities between -10 and +10 km/s, asymmetries northern/southern and other anomalies. The observed features are sensitive to internal and external forces, especially at the largest Galactocentric distances. Here we review some of the Galactic dynamics hypotheses that explain these anomalies: either in terms of gravitational interaction, magnetic fields, accretion of intergalactic matter or others. The gravitational interaction may be among the different components of the Galaxy or…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Astro and Planetary Science
