The dust and gas content of carbon stars toward the Galactic Halo
Eric Lagadec, Greg.C. Sloan, Albert.A. Zijlstra, Nicolas Mauron, J. R., Houck

TL;DR
This study analyzes the dust and gas properties of four carbon stars in the Galactic Halo using Spitzer IRS spectra, revealing their metal-poor gas characteristics but metal-rich dust features, with implications for their origins.
Contribution
First detailed infrared spectral analysis of halo carbon stars showing their dust and gas properties and discussing their possible origins.
Findings
Gas properties indicate metal-poor stars with low expansion velocities.
Dust features suggest these stars may be metal-rich or produce silicon.
The origin of these stars could be from the halo, satellite galaxies, or the galactic disk.
Abstract
We present Spitzer IRS spectra of four carbon stars located in the Galactic Halo and the thick disc. The spectra display typical features of carbon stars with SiC dust emission and CH molecular absorption. Dust radiative transfer models and infrared colors enable us to determine the dust production rates for these stars whilst prior CO measurements yield expansion velocities and total mass-loss rates. The gas properties (low expansion velocities (around 7 km/s) and strong CH molecular absorption bands) are consistent with the stars being metal-poor. However the dust content of these stars (strong SiC emission bands) is very similar to what is observed in metal-rich carbon stars. The strong SiC emission may indicate that the carbon stars derive from a metal-rich population, or that these AGB stars produce silicon. The origin of the halo carbon stars is not known. They…
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