  The relativistic analogue of the Hall-Vinen-Bekarevich-Khalatnikov (HVBK)
hydrodynamics is derived making use of the phenomenological method similar to
that used by Bekarevich and Khalatnikov [1] in their derivation of
HVBK-hydrodynamics. The resulting equations describe a finite-temperature
superfluid liquid with the distributed vorticity. The main dissipative effects,
including mutual friction, are taken into account. The proposed hydrodynamics
is needed for reliable modeling of the dynamical properties of superfluid
neutron stars.

General Relativity and Quantum Cosmology;High Energy Astrophysical Phenomena;Superconductivity