Impact of stellar winds on the pair-instability supernova rate
Fuente:
arXiv
Guardado en:
| Autores principales: | Simonato, Filippo, Torniamenti, Stefano, Mapelli, Michela, Iorio, Giuliano, Boco, Lumen, De Domenico-Langer, Franca, Sgalletta, Cecilia |
|---|---|
| Formato: | Preprint |
| Publicado: |
2025
|
| Materias: | |
| Acceso en línea: | |
| Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
Optically thick winds of very massive stars suppress intermediate-mass black hole formation
por: Torniamenti, Stefano, et al.
Publicado: (2025)
por: Torniamenti, Stefano, et al.
Publicado: (2025)
The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers
por: Sgalletta, Cecilia, et al.
Publicado: (2024)
por: Sgalletta, Cecilia, et al.
Publicado: (2024)
Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
por: Dall'Amico, Marco, et al.
Publicado: (2025)
por: Dall'Amico, Marco, et al.
Publicado: (2025)
Binary black hole mergers from Population III star clusters
por: Mestichelli, Benedetta, et al.
Publicado: (2024)
por: Mestichelli, Benedetta, et al.
Publicado: (2024)
The role of accretion efficiency, natal kicks, and angular momentum transport in the formation of the Gaia black holes
por: Mapelli, Michela, et al.
Publicado: (2026)
por: Mapelli, Michela, et al.
Publicado: (2026)
Impact of gas hardening on the population properties of hierarchical black hole mergers in AGN disks
por: Vaccaro, M. Paola, et al.
Publicado: (2023)
por: Vaccaro, M. Paola, et al.
Publicado: (2023)
A new prescription for the spectral properties of population III stellar populations
por: Lecroq, Marie, et al.
Publicado: (2025)
por: Lecroq, Marie, et al.
Publicado: (2025)
The impact of envelope binding energies on the merger rate density of binary compact objects
por: Sgalletta, Cecilia, et al.
Publicado: (2026)
por: Sgalletta, Cecilia, et al.
Publicado: (2026)
Impact of initial mass function on the chemical evolution of high-redshift galaxies
por: Liu, Boyuan, et al.
Publicado: (2025)
por: Liu, Boyuan, et al.
Publicado: (2025)
The cosmic rate of Pair-Instability Supernovae
por: Gabrielli, Francesco, et al.
Publicado: (2024)
por: Gabrielli, Francesco, et al.
Publicado: (2024)
Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift
por: Torniamenti, Stefano, et al.
Publicado: (2024)
por: Torniamenti, Stefano, et al.
Publicado: (2024)
The boring history of Gaia BH3 from isolated binary evolution
por: Iorio, Giuliano, et al.
Publicado: (2024)
por: Iorio, Giuliano, et al.
Publicado: (2024)
The pair-instability origin of supernova 2023vbw
por: Hiramatsu, Daichi, et al.
Publicado: (2026)
por: Hiramatsu, Daichi, et al.
Publicado: (2026)
Binary black hole mergers from Population III stars: uncertainties from star formation and binary star properties
por: Santoliquido, Filippo, et al.
Publicado: (2023)
por: Santoliquido, Filippo, et al.
Publicado: (2023)
Population synthesis of Be X-ray binaries in the Small Magellanic Cloud: angular momentum recycling and stable mass transfer
por: Oller, Víctor López, et al.
Publicado: (2026)
por: Oller, Víctor López, et al.
Publicado: (2026)
Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars
por: Mestichelli, Benedetta, et al.
Publicado: (2025)
por: Mestichelli, Benedetta, et al.
Publicado: (2025)
Teen TITANS simulations -- I. Inefficient intermediate-mass black hole seeding via stellar collisions in young massive clusters
por: Mestichelli, Benedetta, et al.
Publicado: (2026)
por: Mestichelli, Benedetta, et al.
Publicado: (2026)
The rates and host galaxies of pair-instability supernovae through cosmic time: Predictions from BPASS and IllustrisTNG
por: Briel, Max M., et al.
Publicado: (2024)
por: Briel, Max M., et al.
Publicado: (2024)
The black hole - pair instability boundary for high stellar rotation
por: Winch, Ethan R. J., et al.
Publicado: (2025)
por: Winch, Ethan R. J., et al.
Publicado: (2025)
A machine learning framework to generate star cluster realisations
por: Prodan, George P., et al.
Publicado: (2024)
por: Prodan, George P., et al.
Publicado: (2024)
The role of migration traps in the formation of binary black holes in AGN disks
por: Vaccaro, Maria Paola, et al.
Publicado: (2025)
por: Vaccaro, Maria Paola, et al.
Publicado: (2025)
Thermal emission from bow shocks. III. Variable diffuse X-ray emission from stellar-wind bow shocks driven by dynamical instabilities
por: Mackey, Jonathan, et al.
Publicado: (2025)
por: Mackey, Jonathan, et al.
Publicado: (2025)
Constraining the Initial-Mass Function via Stellar Transients
por: Gabrielli, Francesco, et al.
Publicado: (2024)
por: Gabrielli, Francesco, et al.
Publicado: (2024)
Star-Black Hole Interactions in Young Star Clusters
por: Rastello, Sara, et al.
Publicado: (2025)
por: Rastello, Sara, et al.
Publicado: (2025)
Micro-Tidal Disruption Events in Young Star Clusters
por: Rastello, Sara, et al.
Publicado: (2025)
por: Rastello, Sara, et al.
Publicado: (2025)
Cascading from the winds to the disk: the universality of supernovae-driven turbulence in different galactic interstellar media
por: Connor, Isabelle, et al.
Publicado: (2025)
por: Connor, Isabelle, et al.
Publicado: (2025)
A dust condensation instability in AGN atmospheres: failed winds and the broad line region
por: Owen, James E., et al.
Publicado: (2025)
por: Owen, James E., et al.
Publicado: (2025)
Effective supernova dust yields from rotating and non-rotating stellar progenitors
por: Otaki, Koki, et al.
Publicado: (2025)
por: Otaki, Koki, et al.
Publicado: (2025)
The formation and stability of a cold disc made out of stellar winds in the Galactic Centre
por: Calderón, Diego, et al.
Publicado: (2024)
por: Calderón, Diego, et al.
Publicado: (2024)
Semi-empirical Models of Galaxy Formation and Evolution
por: Lapi, Andrea, et al.
Publicado: (2025)
por: Lapi, Andrea, et al.
Publicado: (2025)
Evidence for the evolution of black hole mass function with redshift
por: Rinaldi, Stefano, et al.
Publicado: (2023)
por: Rinaldi, Stefano, et al.
Publicado: (2023)
Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
por: Dall'Amico, Marco, et al.
Publicado: (2023)
por: Dall'Amico, Marco, et al.
Publicado: (2023)
Repopulating the pair-instability mass gap without sustained growth to massive IMBHs: the case of 47\,Tuc
por: Chattopadhyay, Debatri, et al.
Publicado: (2026)
por: Chattopadhyay, Debatri, et al.
Publicado: (2026)
Accretion rates of stellar-mass compact objects embedded in AGN discs
por: Jiao, Cheng-Liang, et al.
Publicado: (2025)
por: Jiao, Cheng-Liang, et al.
Publicado: (2025)
Wolf-Rayet -- compact object binaries as progenitors of binary compact objects
por: Korb, Erika, et al.
Publicado: (2024)
por: Korb, Erika, et al.
Publicado: (2024)
How do supernova remnants cool? II. Machine learning analysis of supernova remnant simulations
por: Smirnova, P., et al.
Publicado: (2024)
por: Smirnova, P., et al.
Publicado: (2024)
Kinetic simulations of the cosmic ray pressure anisotropy instability: cosmic ray scattering rate in the saturated state
por: Sun, Xiaochen, et al.
Publicado: (2024)
por: Sun, Xiaochen, et al.
Publicado: (2024)
Radio-AGN activity across the galaxy population: dependence on stellar mass, star-formation rate, and redshift
por: Kondapally, R., et al.
Publicado: (2024)
por: Kondapally, R., et al.
Publicado: (2024)
Impacts of hydrogen envelope on supernova fallback and the resulting compact remnant masses
por: Shinoda, Kengo, et al.
Publicado: (2025)
por: Shinoda, Kengo, et al.
Publicado: (2025)
Multi-wavelength study of the high Galactic latitude supernova remnant candidate G118.4+37.0 associated with the Calvera pulsar
por: Greco, Emanuele, et al.
Publicado: (2025)
por: Greco, Emanuele, et al.
Publicado: (2025)
Ejemplares similares
-
Optically thick winds of very massive stars suppress intermediate-mass black hole formation
por: Torniamenti, Stefano, et al.
Publicado: (2025) -
The more accurately the metal-dependent star formation rate is modeled, the larger the predicted excess of binary black hole mergers
por: Sgalletta, Cecilia, et al.
Publicado: (2024) -
Impact of accretion-induced chemically homogeneous evolution on stellar and compact binary populations
por: Dall'Amico, Marco, et al.
Publicado: (2025) -
Binary black hole mergers from Population III star clusters
por: Mestichelli, Benedetta, et al.
Publicado: (2024) -
The role of accretion efficiency, natal kicks, and angular momentum transport in the formation of the Gaia black holes
por: Mapelli, Michela, et al.
Publicado: (2026)