3D spectroscopic analysis of helium-line white dwarfs

TL;DR

This study applies 3D atmospheric models to correct spectroscopic parameters of helium-line white dwarfs, revealing significant adjustments in temperature and gravity, and emphasizing the importance of improved microphysics in atmospheric modeling.

Contribution

Introduces 3D atmospheric corrections for DB and DBA white dwarfs, improving accuracy over traditional 1D models and highlighting the need for better microphysical descriptions.

Findings

3D corrections significantly affect T_eff and log(g) estimates

Corrections are most significant for T_eff < 18000 K

Results align with Gaia DR2 flux measurements within uncertainties

Abstract

In this paper, we present corrections to the spectroscopic parameters of DB and DBA white dwarfs with -10.0 < log(H/He) < -2.0, 7.5 < log(g) < 9.0 and 12000 K < T_eff < 34000 K, based on 282 3D atmospheric models calculated with the CO5BOLD radiation-hydrodynamics code. These corrections arise due to a better physical treatment of convective energy transport in 3D models when compared to the previously available 1D model atmospheres. By applying the corrections to an existing SDSS sample of DB and DBA white dwarfs, we find significant corrections both for the effective temperature and surface gravity. The 3D log(g) corrections are most significant for T_eff < 18000 K, reaching up to -0.20 dex at log(g) = 8.0. However, in this low effective temperature range, the surface gravity determined from the spectroscopic technique can also be significantly affected by the treatment of the neutral van der Waals line broadening of helium and by non-ideal effects due to the perturbation of helium by neutral atoms. Thus, by removing uncertainties due to 1D convection, our work showcases the need for improved description of microphysics for DB and DBA model atmospheres. Overall, we find that our 3D spectroscopic parameters for the SDSS sample are generally in agreement with Gaia DR2 absolute fluxes within 1-3{\sigma} for individual white dwarfs. By comparing our results to DA white dwarfs, we have determined that the precision and accuracy of DB/DBA atmospheric models are similar. For ease of user application of the correction functions, we provide an example Python code.