CS peak fractional abundances of 1-4e-6 and e-folding radii of 1.8-6.8e16 cm are derived for five carbon-rich AGB stars, showing no major differences from IRC+10216 beyond density effects and matching chemical model predictions.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2025 1verdicts
ACCEPT 1representative citing papers
citing papers explorer
-
Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. II. Abundances and spatial distributions of CS
CS peak fractional abundances of 1-4e-6 and e-folding radii of 1.8-6.8e16 cm are derived for five carbon-rich AGB stars, showing no major differences from IRC+10216 beyond density effects and matching chemical model predictions.