High-energy astrophysics
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- Line-of-Sight Acceleration-driven waveform corrections for unequal-mass compact binary coalescences
- Predicting High-Energy neutrino emission from X-ray absorption in CSM-interacting SNe
- Line-of-sight Acceleration Driven Effects in Eccentric Compact Binary Coalescences
- X-ray spectral scaling of black hole mass in quasi-periodic eruptive source RX J1301.9+2747
- Evolution of neutrino distributions under repeated electron scattering
- Does Diffusive Shock Acceleration Reach Steady State? Insights from a Near-Sun Shock Observed by Parker Solar Probe
- Scalable and sequential inference of the neutron star equation of state with the Einstein Telescope
- From the Milky Way to the Early Universe: How Metallicity Shapes the Formation of Double Neutron Stars
- Pulsations and constraints on time lags in two distinct ULXs: NGC 5204 X-1 and NGC 55 ULX-1
- Deep radio characterization of the supernova remnant G343.1-00.7
- Radio and X-ray Observations of the Transitional Supernova 2019yvr: Insights into the Progenitor Mass-Loss History
- Beta-Particle Transport and Thermalization in Kilonova Ejecta with Detailed Atomic Microphysics
- Detection of relativistic orbital deformation from improved timing of PSR J1757−1854
- Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models
- Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum
- The jet-shaped pipe morphology in planetary nebulae and core-collapse supernova remnants
- Angular momentum drives proton-rich nucleosynthesis in hyperaccreting neutron stars in common envelopes
- First Light of Neutron Star Mergers: Off-axis Cocoon Cooling X-Ray Emission from Short Gamma-Ray Burst Jets
- Detection of Knots in the Type Iax Supernova Remnant Pa 30
- An Optically Motivated Gamma-Ray Study of Fermi-LAT Novae
- Probing turbulence in the ionized interstellar medium using young pulsars. I. Dispersion measure variations
- Reflex instabilities II: The reflex motion of the central object drives at least seven instabilities in accretion discs
- Reflex instabilities I: Boundaries makes grid-based disc simulations frame-dependent
- The Potential Contribution of Radiative Supernova Remnants to the Local Cosmic Ray Spectrum
- The neutrino magnetic moment and supernovae with strong magnetic fields