Simulation-derived Stark-broadened He I profiles are compared to semi-analytical ones for DB white dwarf spectroscopy, including impacts from frequency sampling, neutral particle broadening, and hydrodynamical effects on SDSS DR17 data.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.SR 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Wide WD+MS binaries from Gaia show large intrinsic scatter in [Fe/H] at all ages for the Galactic disk AMR, agreeing with prior studies and indicating complex chemical evolution.
citing papers explorer
-
A Theoretical Investigation of He I Line Profiles for the Spectroscopic Analysis of DB White Dwarfs
Simulation-derived Stark-broadened He I profiles are compared to semi-analytical ones for DB white dwarf spectroscopy, including impacts from frequency sampling, neutral particle broadening, and hydrodynamical effects on SDSS DR17 data.
-
Revisiting the Galactic age-metallicity relation from wide white dwarf-main-sequence binaries
Wide WD+MS binaries from Gaia show large intrinsic scatter in [Fe/H] at all ages for the Galactic disk AMR, agreeing with prior studies and indicating complex chemical evolution.