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Constraining the Geometry of Galactic Dark Matter with Gaia Data Release 3

  • Authors: Francesco Sylos Labini, Roberto Capuzzo-Dolcetta

Francesco Sylos Labini and Roberto Capuzzo-Dolcetta 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 8.

Best fit of the DM disk model to the rotation curves (top panel) and corresponding behavior of the vertical acceleration (bottom panel), computed assuming a mean vertical scale height of ﹩\overline{{z}_{\,\rm{d}\,}}=0.22\pm 0.04﹩ kpc.

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