A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp star alpha Circini

Details A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp star alpha Circini A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp star alpha Circini

2009-03-20

arxiv.org/abs/0903.3512v1

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

14 pages, 11 figures; accepted for publication in Astronomy & Astrophysics

Scientific paper

Chemically peculiar (CP) stars are unique natural laboratories for investigation of the microscopic diffusion processes of chemical elements. The element segregation under the influence of gravity and radiation pressure leads to the appearance of strong abundance gradients in the atmospheres of CP stars. Consequently, the atmospheric temperature-pressure structure of these objects could deviate significantly from the atmospheres of normal stars with homogeneous abundances. In this study we performed a self-consistent, empirical model atmosphere study of the brightest rapidly oscillating Ap star alpha Cir. We account for chemical stratification in the model atmosphere calculations and assess the importance of non-uniformed vertical element distribution on the model structure, energy distribution and hydrogen line profiles. Based on an iterative procedure of the chemical abundance analysis of 52 ions of 35 elements, stratification modeling of 4 elements (Si, Ca, Cr and Fe) and subsequent re-calculations of the atmospheric structure, we derived a new model atmosphere of alpha Cir, which is consistent with the inferred atmospheric chemistry of the star. We find Teff=7500 K, logg=4.1, and demonstrate that chemical stratification has a noticeable impact on the model structure and modifies the formation of the hydrogen Balmer lines. Our spectroscopically determined Teff of alpha Cir agrees with the fundamental effective temperature of this star. This shows that temperatures inferred in detailed spectroscopic analyses of cool magnetic CP stars are not affected by a large systematic bias.

Affiliated with

Also associated with

No associations

Rating

A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp star alpha Circini does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp star alpha Circini, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A self-consistent empirical model atmosphere, abundance and stratification analysis of the benchmark roAp star alpha Circini will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-642082