Anisotropic String Cosmological Models in Heckmann-Suchuking Space-Time
  In the present work we have searched the existence of the late time acceleration of the universe with string fluid as source of matter in anisotropic Heckmann-Suchking space-time by using 287 high red shift $(0.3 \leq z\leq 1.4)$ SN Ia data of observed absolute magnitude along with their possible error from Union 2.1 compilation. It is found that the best fit values for $(\Omega_{m})_{0}$, $(\Omega_{\Lambda})_{0}$, $(\Omega_{\sigma})_{0}$ and $(q)_{0}$ are 0.2820, 0.7177, 0.0002 $\&$ -0.5793 respectively. Several physical aspects and geometrical properties of the model are discussed in detail. 
G. K. Goswami, R. N. Dewangan, A. K. Yadav and A. Pradhan
gr-qc