ZTF-discovered radial-mode sdB pulsators have mean Teff of 28,300 K and log g of 5.56, placing them at the boundary between V361 Hya and V1093 Her classes with canonical masses and distinguishing them from blue large-amplitude pulsators.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Flux-resolved NuSTAR spectra of 4U 0115+63 show the 10 keV feature maintains constant centroid energy while its flux ratio to the continuum anticorrelates with overall flux, indicating a formation mechanism distinct from both the broadband continuum and the CRSF harmonics.
citing papers explorer
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Spectroscopic follow-up of hot subdwarf variables found in ZTF -- Atmospheric and fundamental properties of radial-mode sdB pulsators
ZTF-discovered radial-mode sdB pulsators have mean Teff of 28,300 K and log g of 5.56, placing them at the boundary between V361 Hya and V1093 Her classes with canonical masses and distinguishing them from blue large-amplitude pulsators.
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Flux variability of the "10 keV feature" of 4U 0115+63
Flux-resolved NuSTAR spectra of 4U 0115+63 show the 10 keV feature maintains constant centroid energy while its flux ratio to the continuum anticorrelates with overall flux, indicating a formation mechanism distinct from both the broadband continuum and the CRSF harmonics.