A research team led by Prof. Jiao Chengliang at the Yunnan Observatories of the Chinese Academy of Sciences, along with collaborators, has introduced a self-consistent model that addresses long-unresolved theoretical gaps in the study of self-gravitating spherical accretion. The study was recently published in The Astrophysical Journal.



Summary

A team led by Prof. Jiao Chengliang has developed a new, self-consistent model for spherical accretion, tackling long-standing theoretical challenges. This model, published in The Astrophysical Journal, focuses on self-gravitating scenarios, providing a more complete understanding of how matter accretes onto celestial objects. By creating a self-consistent framework, the researchers bridge previous theoretical gaps, offering a more accurate depiction of this fundamental astrophysical process. This advancement enhances our understanding of phenomena like star formation and black hole growth.

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