2024
DOI: 10.3847/1538-4357/ad6dd4
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Radiation Hydrodynamic Simulations of Massive Stars in Gas-rich Environments: Accretion of AGN Stars Suppressed by Thermal Feedback

Yi-Xian 逸贤 Chen 陈,
Yan-Fei 燕飞 Jiang 姜,
Jeremy Goodman
et al.

Abstract: Massive stars may form in or be captured into active galactic nuclei (AGN) disks. Recent 1D studies employing stellar-evolution codes have demonstrated the potential for rapid growth of such stars through accretion up to a few hundred solar masses. We perform 3D radiation hydrodynamic simulations of moderately massive stars’ envelopes in order to determine the rate and critical radius R crit of their accretion process in an isotropic gas-rich environment in the absence of luminosity-driven ma… Show more

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