Exact Solution of a (2+1)-Dimensional Anisotropic Star in Finch and Skea Spacetime

We provide a new class of interior solution of a (2+1)-dimensional anisotropic star in Finch and Skea spacetime corresponding to the BTZ black hole. We develop the model by considering the MIT bag model EOS and a particular ansatz for the metric function g_rr proposed by Finch and Skea [M.R. Finch and J.E.F. Skea, Class. Quantum. Grav. 6 (1989) 467]. Our model is free from central singularity and satisfies all the physical requirements for the acceptability of the model.