Numerical models of neutron star atmospheres from fusion ashes show a radiation-pressure layer limiting flux and absorption edges tied to chemical composition, with fits to diluted blackbodies plus edges for X-ray burst interpretation.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Shocks in the hottest galaxy clusters produce observable Z/W ratios in the Fe XXV triplet and ion-temperature line broadening that can constrain electron heating and temperature equilibration with XRISM.
citing papers explorer
-
Neutron star atmospheres composed of fusion ashes
Numerical models of neutron star atmospheres from fusion ashes show a radiation-pressure layer limiting flux and absorption edges tied to chemical composition, with fits to diluted blackbodies plus edges for X-ray burst interpretation.
-
Iron He-triplet signatures of shocks in the hottest galaxy clusters. Z/W line ratio, line broadening, and electron-ion temperature equilibration
Shocks in the hottest galaxy clusters produce observable Z/W ratios in the Fe XXV triplet and ion-temperature line broadening that can constrain electron heating and temperature equilibration with XRISM.