| Issue |
EAS Publications Series
Volume 71-72, 2015
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
|
|
|---|---|---|
| Page(s) | 195 - 196 | |
| Section | Binaries | |
| DOI | https://doi.org/10.1051/eas/1571044 | |
| Published online | 01 December 2015 | |
The Physics of Evolved Stars: A Conference Dedicated to the Memory of Olivier Chesneau
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 195-196
E. Lagadec, F. Millour and T. Lanz (eds)
EAS Publications Series, 71–72 (2015) 195-196
Indication of The High Mass-Transfer Ratio In S-Type Symbiotic Binaries
Astronomical Institute of the Slovak Academy of Sciences, Tatranská Lomnica, Slovakia
By modelling H0 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.
© EAS, EDP Sciences, 2015