Fig. 4.
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Integrated orbits of DQ Hya (thick solid line: distance from parallax inversion; dashed line: distance estimated from the RR Lyrae magnitude–metallicity relation) and ASAS J153830–6906.4 (thin solid line: distance from parallax inversion), computed using the Milky Way potential models by McMillan (2017, M17, left panel) and Allen & Santillan (1991, AS91, right panel).
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