Characterizing the Bolometric-photoevaporative Transition in Young Sub-Neptunes with Radiation-hydrodynamic Simulations

William Misener, Matthäus Schulik, Hilke E. Schlichting, James E. Owen

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DOI: 10.3847/1538-4357/ae969c
Published: 2026-09-02
Container: The Astrophysical Journal
Publisher: American Astronomical Society
Open access: unknown

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Cite this work

BibTeX

@article{allodium:10.3847/1538-4357/ae969c,
  title = {Characterizing the Bolometric-photoevaporative Transition in Young Sub-Neptunes with Radiation-hydrodynamic Simulations},
  author = {William Misener and Matthäus Schulik and Hilke E. Schlichting and James E. Owen},
  year = {2026},
  journal = {The Astrophysical Journal},
  doi = {10.3847/1538-4357/ae969c},
  url = {https://doi.org/10.3847/1538-4357/ae969c}
}

RIS

TY  - JOUR
TI  - Characterizing the Bolometric-photoevaporative Transition in Young Sub-Neptunes with Radiation-hydrodynamic Simulations
AU  - William Misener
AU  - Matthäus Schulik
AU  - Hilke E. Schlichting
AU  - James E. Owen
PY  - 2026
JO  - The Astrophysical Journal
DO  - 10.3847/1538-4357/ae969c
UR  - https://doi.org/10.3847/1538-4357/ae969c
ER  -

APA

Misener, W., Schulik, M., Schlichting, H. E., & Owen, J. E. (2026). Characterizing the Bolometric-photoevaporative Transition in Young Sub-Neptunes with Radiation-hydrodynamic Simulations. The Astrophysical Journal. https://doi.org/10.3847/1538-4357/ae969c

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crossref · retrieved 2026-09-25T19:59:03.526Z