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To explain the reason of accelerated expansion of our universe dark energy isa suitable candidate. Motivated by this concept in the present paper we haveobtained a new model of an anisotropic superdense star which admits conformalmotions in presence of quintessence field which is characterized by a parameter$omega$ with omega lies in the range -1 to -1/3.The model has been developed bychoosing Vaidya-Titekar ansatz [P C Vaidya and R Tikekar (1982)J. Astrophys.Astron. 3 325].Our model satisfy all the physical requirements.We have analyzeour result analytically as well as with the help of graphical representation.

Vaidya-Tikekar Type Superdense Star Admitting Conformal Motion in Presence of Quintessence Field