Matches in SemOpenAlex for { <https://semopenalex.org/work/W2001504455> ?p ?o ?g. }
- W2001504455 abstract "Caustic rings of dark matter were predicted to exist in the plane of the Galaxy at radii ${a}_{n}ensuremath{simeq}40text{ }text{ }mathrm{kpc}/n$ for $n=1,2,3,dots{}$. The recently discovered Monoceros Ring of stars is located near the $n=2$ caustic, prompting us to consider a possible connection between these two objects. We identify two processes through which the Monoceros Ring of stars may have formed. One process is the migration of gas to an angular velocity minimum at the caustic leading to enhanced star formation there. The other is the adiabatic deformation of star orbits as the caustic slowly grows in mass and radius. The second process predicts an order 100% enhancement of the density of disk stars at the location of the caustic ring." @default.
- W2001504455 created "2016-06-24" @default.
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- W2001504455 date "2007-07-10" @default.
- W2001504455 modified "2023-10-18" @default.
- W2001504455 title "Does the second caustic ring of dark matter cause the Monoceros Ring of stars?" @default.
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- W2001504455 doi "https://doi.org/10.1103/physrevd.76.023505" @default.
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