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Stellar model chromospheres. V. Alpha Centauri A (G2 V) and alpha Centauri B (Kl V)

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/154818· OSTI ID:7240241
We propose models for the upper photospheres and lower chromospheres of ..cap alpha.. Cen A and B based on a partial redistribution (PRD) analysis of the Ca II K line cores and damping wings. Coude spectrograms of the Ca II regions in these stars obtained with the Mount Stromlo 74 inch (1.9 m) telescope are calibrated by fitting the far wing profiles of K with synthetic fluxes based on radiative equilibrium (RE) models. The RE calibrations are verified by comparison with independent calibrations using Willstrop's absolute photometry and narrow band fluxes obtained at Mount Stromlo. Deviations of the empirical profiles from the RE fluxes in the inner wings of K suggest departures from radiative equilibrium in the upper photosphere of ..cap alpha.. Cen A comparable to those found previously for the Sun and Procyon. Alpha Cen B shows similar departures from RE when the effects of CO cooling near the temperature minimum are taken into account. We find similar ratios of T/sub min//T/sub eff/ for both stars, which are within the range of T/sub min//T/sub eff/ ratios determined previously for the Sun, Procyon, and Arcturus. In addition, we find similar mass column densities at the 8000 K levels of the ..cap alpha.. Cen A and B chromospheres comparable to those determined for the Sun and Procyon. Finally, ..cap alpha.. Cen A appears to be more evolved and possibly much older than the Sun, despite its similar chromosphere structure. (AIP)
Research Organization:
Joint Institute for Laboratory Astrophysics, University of Colorado and National Bureau of Standards
OSTI ID:
7240241
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 210:1; ISSN ASJOA
Country of Publication:
United States
Language:
English

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