Indication of the High Mass-Transfer Ratio in S-type Symbiotic Binaries
classification
🌌 astro-ph.SR
keywords
s-typesymbioticwindanalysisbinariescolumncorrespondingdensities
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By modelling H$^0$ column densities in eclipsing S-type symbiotic stars EG And and SY Mus, we derived the wind velocity profile and the corresponding mass-loss rate from their giants. Our analysis revealed a strong enhancement of the wind at the orbital plane.
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