Rapid Stellar and Binary Population Synthesis with COMPAS: Methods Paper II

Abstract The COMPAS ( https://compas.science ) public rapid binary population synthesis code has undergone a number of key improvements since the original COMPAS methods paper was published. These include more sophisticated and robust treatments of binary interactions: mass transfer physics; common-envelope events; tides and gravitational-wave radiation reaction; and updated prescriptions for stellar evolution, winds, and supernovae. The code structure and outputs have also been updated, with a focus on improving resolution without sacrificing computational speed. This paper describes the substantive changes in the code between the previous methods paper and COMPAS v03.22.01.

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Publication Details

Journal
The Astrophysical Journal Supplement Series
Published
2025-09-01
DOI
https://doi.org/10.3847/1538-4365/adf8d0
Citations
4
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
4.62

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article

Rapid Stellar and Binary Population Synthesis with COMPAS: Methods Paper II

Mike Y. M. Lau, A. Vajpeyi, Veome Kapil, Nicolás Rodríguez-Segovia et al.
4 citations
The Astrophysical Journal Supplement Series
Stellar, planetary, and galactic studies
4.62
article

Rapid Stellar and Binary Population Synthesis with COMPAS: Methods Paper II

Mike Y. M. Lau, A. Vajpeyi, Veome Kapil, Nicolás Rodríguez-Segovia, Ilya Mandel, I. M. Romero-Shaw, Jeff Riley, Ryosuke Hirai, L. A. C. van Son, Reinhold Willcox, J. Merritt, Alejandro Vigna-Gómez, Adam Boesky, S. P. Stevenson, Y. Song, Adam Brček
article en
4 citations

Abstract

Abstract The COMPAS ( https://compas.science ) public rapid binary population synthesis code has undergone a number of key improvements since the original COMPAS methods paper was published. These include more sophisticated and robust treatments of binary interactions: mass transfer physics; common-envelope events; tides and gravitational-wave radiation reaction; and updated prescriptions for stellar evolution, winds, and supernovae. The code structure and outputs have also been updated, with a focus on improving resolution without sacrificing computational speed. This paper describes the substantive changes in the code between the previous methods paper and COMPAS v03.22.01.

The Astrophysical Journal Supplement SeriesVol. 280(1)
Australian Research Council (AU), Pioneer (United States) (US), Johns Hopkins University (US), University of Auckland (NZ), University of Oregon (US), Princeton University (US), University of Cambridge (GB), UNSW Sydney (AU), Australian Defence Force Academy (AU), Max Planck Institute for Astrophysics (DE), Institute of Astronomy (RU), Center for Astrophysics Harvard & Smithsonian (US), ARC Centre of Excellence for Gravitational Wave Discovery (AU), Flatiron Health (United States) (US), Bristol Robotics Laboratory (GB), Flatiron Institute (US), Monash University (AU), Swinburne University of Technology (AU), Heidelberg Institute for Theoretical Studies (DE), KU Leuven (BE)
National Science Foundation, National Aeronautics and Space Administration, Aspen Center for Physics, Astronomy Australia Limited, New Zealand Government, Royal Society Te Apārangi, Swinburne University of Technology, Science and Technology Facilities Council, Marsden Fund
Openalex Percentile: Top 5%
Stellar, planetary, and galactic studies
4.62
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