A5044924988- Astronomy and Astrophysical Research
- Stellar, planetary, and galactic studies
- Radio Astronomy Observations and Technology
- Galaxies: Formation, Evolution, Phenomena
- Gamma-ray bursts and supernovae
- Pulsars and Gravitational Waves Research
- Solar and Space Plasma Dynamics
Nicolaus Copernicus University
2023
Institute of Space Technology
2019
Stars strongly impact their environment, and shape structures on all scales throughout the universe, in a process known as ``feedback''. Due to complexity of both stellar evolution physics larger astrophysical structures, there remain many unanswered questions about how feedback operates, what we can learn stars by studying imprint wider universe. In this white paper, summarize discussions from Lorentz Center meeting `Bringing Stellar Evolution Feedback Together' April 2022, identify key...
Stars strongly impact their environment, and shape structures on all scales throughout the universe, in a process known as ``feedback''. Due to complexity of both stellar evolution physics larger astrophysical structures, there remain many unanswered questions about how feedback operates, what we can learn stars by studying imprint wider universe. In this white paper, summarize discussions from Lorentz Center meeting `Bringing Stellar Evolution Feedback Together' April 2022, identify key...
Numerous galaxies host a massive black hole (MBH) in their galactic nuclei enclosed by dense stellar population. extreme mass-ratio inspirals (EMRIs) and intermediate (IMRIs) are the most compelling sources of gravitational radiation detectable laser interferometer space antenna (LISA) that will have capability to observe entire sky probe Universe. EMRIs IMRIs prime source for LISA encompasses whirling COs, typically stellar-mass holes (BH), neutron stars (NS), white dwarfs (WD) mass (IMBH)...