constructed by applying the cut-and-paste technique to two copies of such black holes. We analyzed various as- pects of this wormhole, such as the amount of exotic matter required, the attractive or repulsive nature of the wormhole, and a possible equation of state for the thin shell. The stability analysis concentrated on the parame- ter β , normally interpreted as the speed of sound. It was found that whenever the two event horizons are close to- gether, a stability region exists for some values of β 2 less than unity, unlike the the cases discussed in Refs. [2] and [19] for Schwarzschild and dilaton thin-shell wormholes, respectively. AAU, FR and SR are thankful to Inter-University Cen- tre for Astronomy and Astrophysics, Pune, India for pro- viding Visiting Associateship under which a part of this work is carried out. FR and ZH are also grateful to UGC, Govt. of India and D.S. Kothari fellowship, for financial support. Acknowledgments 6 [22] T.A. Roman, Phys. Rev. D 53 , (1993) 5496. [11] E. Eiroa and C. Simeone, Phys. Rev. D 76 , (2007) 024021. [10] F. Rahaman et al., Gen. Rel. Grav. 38 , (2006) 1687. [9] F.S.N. Lobo, Phys. Rev. D 71 , (2005) 124022. [8] M. Thibeault, C. Simeone and E.F. Eiroa, Gen. Rel. Grav. 38 , (2006) 1593. [7] E.F. Eiroa and C. Simeone, Phys. Rev. D 71 , (2005) 127501. [6] E.F. Eiroa and C. Simeone, Phys. Rev. D 70 , (2004) 044008. [4] F.S.N. Lobo, Class. Quant. Grav. 21 , (2004) 4811. [5] E.F. Eiroa and G. Romero, Gen. Rel. Grav. 36 , (2004) 651. [3] F.S.N. Lobo and P. Crawford, Class. Quant. Grav. 21 , (2004) 391. [2] E. Poisson and M. Visser, Phys. Rev. D 52 , (1995) 7318. [1] M. Visser, Nucl. Phys. B 328 , (1989) 203. [21] S. Sur, S. Das, and S. SenGupta, JHEP 0510 , (2005) 064. [20] E.F. Eiroa, M.G. Richarte, and C. Simeone, Phys. Lett. A 373 (2008) 1. [19] E.F. Eiroa, Phys. Rev. D 78 , (2008) 024018. [18] F. Rahaman et al., Mod. Phys. Lett. A 24 , (2009) 53. [17] F. Rahaman et al., Acta Phys. Polon. B 40 , (2009) 1575. [16] M. G. Richarte and C. Simeone, Phys. Rev. D 76 , (2007) 087502. [15] J. P. S. Lemos and F.S.N. Lobo, Phys. Rev. D 78 , (2008) 044030. [14] F. Rahaman et al., Chin. J. Phys. 45 , (2007) 518. [13] F. Rahaman et al., Gen. Rel. Grav. 39 , (2007) 945. [12] F. Rahaman et al., Int. J. Mod. Phys. D 16 , (2007) 1669.