The Fe K line of GX 340+0 shows a dual-peaked structure with residual narrow emission features at the ~5% level that RELXILLNS reflection modeling alone does not reproduce.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
The Structure of the Relativistic Fe Line in GX 340+0 as Viewed with XRISM/Resolve, NICER, and NuSTAR
The Fe K line of GX 340+0 shows a dual-peaked structure with residual narrow emission features at the ~5% level that RELXILLNS reflection modeling alone does not reproduce.