NLTE spectral analysis of the intermediate helium-rich subdwarf B star CPD-20{\deg}1123
L. L\"obling

TL;DR
This paper analyzes the intermediate helium-rich subdwarf B star CPD-20{ extdegree}1123 using NLTE stellar atmosphere models, providing insights into its atmospheric composition and testing the NLTE modeling approach at high temperatures.
Contribution
It presents the first application of revised model atoms for light metals with the NLTE atmosphere code and tests the code's validity at high temperatures.
Findings
He/H ratio of 0.13 ± 0.05 in CPD-20{ extdegree}1123
Effective temperature of 25,500 ± 1,000 K and log g of 5.3 ± 0.3
Validation of NLTE models for intermediate He-rich sdB stars
Abstract
Subdwarf B (sdB) stars are core helium-burning stars with stratified atmospheres. Their atmospheres are dominated by hydrogen (H) while the helium (He) and metal abundances are shaped by an interplay of gravitational settling and radiative levitation. However, a small fraction of these show spectra dominated by He I absorption lines. In between these groups of He-deficient and extreme He-rich sdBs, some are found to have intermediate surface He abundances. These objects are proposed to be young "normal" (He-deficient) sdBs for which the dynamical stratification of the atmosphere is still ongoing. We present an analysis of the optical spectrum of such an intermediate He-rich sdB, namely CPD-20{\deg}1123, by means of non-local thermodynamic equilibrium (NLTE) stellar atmosphere models. It has a He-to-H number ratio of and its effective temperature of…
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