Abstract
It is quite fascinating to study the low-mass compact stars because of their enigmatic behaviour. In this paper, we have modelled this kind of low-mass strange stars based on the Heintzmann ansatz in $$(2+1)$$ dimensions. Attractive anisotropic force plays a significant role in restricting the upper mass limit (which is comparatively low) of the strange star. We have applied our model to some low-mass strange stars. Our model is useful to predict important parameters of the low-mass strange stars.
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