Connecting stellar and galactic scales: Energetic feedback from stellar wind bubbles to supernova remnants

被引：0
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作者：
Fichtner, Yvonne A. [1 ]
Mackey, Jonathan [2 ]
Grassitelli, Luca [1 ]
Romano-Díaz, Emilio [1 ]
Porciani, Cristiano [1 ,3 ,4 ,5 ]
机构：
[1] Argelander-Institut für Astronomie, Auf dem Hügel 71, Bonn,53121, Germany
[2] Dublin Institute for Advanced Studies, Astronomy and Astrophysics Section, DIAS Dunsink Observatory, Dublin,D15 XR2R, Ireland
[3] SISSA, International School for Advanced Studies, Via Bonomea 265, TS, Trieste,34136, Italy
[4] Dipartimento di Fisica, Sezione di Astronomia, Università di Trieste, Via Tiepolo 11, Trieste,34131, Italy
[5] IFPU, Institute for Fundamental Physics of the Universe, Via Beirut 2, Trieste,34151, Italy
来源：
Astronomy and Astrophysics | 1600年 / 690卷
关键词：
YAF; ERD and CP gratefully acknowledge the Collaborative Research Center 1601 (SFB 1601 sub-projects C5 and C6) funded by the Deutsche Forschungsgemeinschaft (DFG; German Research Foundation) - 500700252. This work was also carried out within the Collaborative Research Centre 956; sub-project C04; funded by the Deutsche Forschungsgemeinschaft (DFG) - project ID 184018867. YAF is part of the International Max Planck research school in Astronomy and Astrophysics and guest at the Max-Planck-Institute for Radio Astronomy. JM acknowledges support from a Royal Society-Science Foundation Ireland University Research Fellowship (20/RS-URF-R/3712). JM is grateful to Prof. N. Langer for the use of a guest office at the AIfA during the time when this research was carried out. CP is grateful to SISSA; the University of Trieste; and IFPU; where part of this work was carried out; for hospitality and support. In addition to the software cited in the main text; this research made use of: the SILO library for data I/O (https://software.llnl.gov/Silo/); the SUNDIALS ODE solver library (Hindmarsh et al. 2005; Gardner et al. 2022); PYPION; (Green; Mackey; 2021); NUMPY (Harris et al. 2020); MATPLOTLIB; (Hunter; 2007); SCIPY (Virtanen et al. 2020); ASTROPY (Astropy Collaboration 2022) and SEABORN (Waskom 2021).YAF; German Research Foundation) u2013 500700252. This work was also carried out within the Collaborative Research Centre 956; funded by the Deutsche Forschungsgemeinschaft (DFG) u2013 project ID 184018867. YAF is part of the International Max Planck research school in Astronomy and Astrophysics and guest at the Max-Planck-Institute for Radio Astronomy. JM acknowledges support from a Royal Society-Science Foundation Ireland University Research Fellowship (20/RS-URF-R/3712). JM is grateful to Prof. N. Langer for the use of a guest office at the AIfA during the time when this research was carried out. CP is grateful to SISSA; this research made use of: the S ILO library for data I/O ( https://software.llnl.gov/Silo/ ); the S UNDIALS ODE solver library (Hindmarsh et al. 2005; N UM P Y (Harris et al. 2020); S CI P Y (Virtanen et al. 2020); A STROPY (Astropy Collaboration 2022) and SEABORN (Waskom 2021);
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