When hadron-quark continuity is formulated in terms of a topology change at a density higher than twice the nuclear matter density (n0), the core of massive compact stars can be described in terms of quasiparticles of fractional baryon charges, behaving neither like pure baryons nor like deconfined quarks. Hidden symmetries, both local gauge and pseudo-conformal (or broken scale), emerge and give rise both to the long-standing "effective g * A ≈ 1" in nuclear Gamow-Teller transitions at ∼ < n0 and to the pseudo-conformal sound velocity v 2 pcs /c 2 ≈ 1/3 at ∼ > 3n0. It is suggested that what has been referred to, since a long time, as "quenched gA" in light nuclei reflects what leads to the dilaton-limit g DL A = 1 at near the (putative) infrared fixed point of scale invariance. These properties are confronted with the recent observations in Gamow-Teller transitions and in astrophysical observations.