Improved determination of the atmospheric parameters of the pulsating sdB star Feige 48

TL;DR

This paper presents an improved spectroscopic analysis of the pulsating sdB star Feige 48 using new NLTE, line-blanketed models, resulting in more accurate atmospheric parameters consistent with previous estimates.

Contribution

The study introduces a refined spectroscopic analysis of Feige 48 with advanced NLTE models and multi-spectral data, enhancing the accuracy of atmospheric parameter determination.

Findings

Derived atmospheric parameters are Teff=29,850 K, log g=5.46, log N(He)/N(H)=-2.88.

First modeling of the He II 1640 Å line confirms optical results.

NLTE effects have a small impact on parameter estimates for Feige 48.

Abstract

As part of a multifaceted effort to exploit better the asteroseismological potential of the pulsating sdB star Feige 48, we present an improved spectroscopic analysis of that star based on new grids of NLTE, fully line-blanketed model atmospheres. To that end, we gathered four high S/N time-averaged optical spectra of varying spectral resolution from 1.0 \AA\ to 8.7 \AA, and we made use of the results of four independent studies to fix the abundances of the most important metals in the atmosphere of Feige 48. The mean atmospheric parameters we obtained from our four spectra of Feige 48 are : Teff= 29,850 $\pm$ 60 K, log $g$ = 5.46 $\pm$ 0.01, and log N(He)/N(H) = $-$2.88 $\pm$ 0.02. We also modeled for the first time the He II line at 1640 \AA\ from the STIS archive spectrum of the star and we found with this line an effective temperature and a surface gravity that match well the values obtained with the optical data. With some fine tuning of the abundances of the metals visible in the optical domain we were able to achieve a very good agreement between our best available spectrum and our best-fitting synthetic one. Our derived atmospheric parameters for Feige 48 are in rather good agreement with previous estimates based on less sophisticated models. This underlines the relatively small effects of the NLTE approach combined with line blanketing in the atmosphere of this particular star, implying that the current estimates of the atmospheric parameters of Feige 48 are reliable and secure.