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The limiting mass is a significant characteristic for compact exotic stars.In the case of quark stars, the limiting mass can be expressed in terms offundamental constants and the Bag constant. In the present work, using bagmodel description, the maximum mass of a rotating quark star is found to dependon the rotational frequency apart from other fundamental parameters. Theanalytical results obtained agree with the results of several relevantnumerical estimates as well as observational evidences.

Chandrasekhar limit for rotating quark stars