Low-mass bare strange stars

R. X. Xu

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arXiv · astro-ph/0410652

Low-mass bare strange stars

R. X. Xu

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Abstract

Strange stars with low masses are suggested to exist in reality, the origin of which could be via accretion-induced collapse (AIC) of white dwarfs. Such a strange star is likely bare, and would thus spin very fast, even to a period of < 0.1 ms. Strange stars with low masses may differ from those with solar-masses in various astrophysical appearances. Observations to test this ``low-mass'' idea are proposed.

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R. X. Xu. 2004-10-27. Low-mass bare strange stars. https://arxiv.org/abs/astro-ph/0410652

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