  In this paper, we construct thin-shell wormholes from regular Ayon-Beato and
Garcia black hole by employing cut and paste formalism and examine their
stability. We analyze attractive and repulsive characteristics of wormholes
corresponding to outward and inward-directed acceleration components,
respectively. A general equation of state is assumed as a linear perturbation
to explore stability of these constructed wormholes with and without
cosmological constant. We consider linear, logarithmic and Chaplygin gas models
for exotic matter and evaluate stability regions for different values of
charge. For horizon-free case, it is found that the generalized Chaplygin gas
model provides maximum stable regions in de Sitter background while the
modified generalized Chaplygin gas and logarithmic gas yield maximum stable
regions in anti-de Sitter spacetime.
