Using heated-envelope white dwarf models in X-ray spectral fitting raises the average intermediate polar white dwarf mass to 0.82 solar masses, matching optical CV values.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
X-ray spectroscopy method of white dwarf mass determination in intermediate polars. External systematic uncertainties
Using heated-envelope white dwarf models in X-ray spectral fitting raises the average intermediate polar white dwarf mass to 0.82 solar masses, matching optical CV values.