Modelling massive star feedback with Monte Carlo radiation hydrodynamics: photoionization and radiation pressure in a turbulent cloud

Author:

Ali Ahmad1ORCID,Harries Tim J1ORCID,Douglas Thomas A1

Affiliation:

1. Department of Physics and Astronomy, University of Exeter, Stocker Road, Exeter EX4 4QL, UK

Funder

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 25 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. 2a Results: galaxy to cloud scales;Frontiers in Astronomy and Space Sciences;2023-11-09

2. The energy and dynamics of trapped radiative feedback with stellar winds;Monthly Notices of the Royal Astronomical Society;2023-09-07

3. Star cluster formation and feedback in different environments of a Milky Way-like galaxy;Monthly Notices of the Royal Astronomical Society;2023-06-29

4. The Effect of Molecular Cloud Properties on the Kinematics of Stars Formed in the Trifid Region;The Astrophysical Journal;2022-09-01

5. Supernovae and photoionizing feedback in spiral arm molecular clouds;Monthly Notices of the Royal Astronomical Society;2022-04-08

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