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Warped and Hooked: Mapping the Magellanic Clouds in Three Dimensions Using Red Clump Stars

  • Authors: Slater J. Oden, David L. Nidever, Joshua Povick, Pol Massana, Yumi Choi, Roeland P. van der Marel, Maria-Rosa L. Cioni, Joanna Sakowska, Knut A. G. Olsen, Lara Cullinane, Danny Horta, Andres Almeida, J. A. Carballo-Bello, D. Crnojević, P. S. Ferguson, C. E. Martínez-Vázquez, G. E. Medina, B. Mutlu-Pakdil, M. Navabi, A. B. Pace, A. H. Riley, Guy S. Stringfellow, A. K. Vivas, David J. James

Slater J. Oden et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 12.

z-coordinate map in the on-sky Cartesian coordinate frame, color coded by the vertical coordinate z (in kiloparsecs). The map is centered on our newly derived RC LMC center (α, δ) = (﹩80\mathop{.}\limits^{^\circ }60﹩, ﹩-69\mathop{.}\limits^{^\circ }80﹩) and a fiducial distance of D0 = 49.15 kpc. Concentric dashed circles indicate angular separations of 7° (∼6 kpc), 10° (∼9 kpc), and 13° (∼11.4 kpc) from the LMC center. A prominent central spiral feature is visible in red, but rapidly dissipates due to the LMC’s disk inclination. At radii ≳ 7°, the peripheral warp becomes strikingly apparent in the vertical structure as blue color.

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