Abstract
We give a brief report on spectroscopic properties of V 393 Scorpii. Ha emission and shape and radial velocity of He I 5875 are modulated with the long cycle. The long cycle is explained as a relaxation cycle in the circumprimary disc, that cumulates the mass transferred from the donor until certain instability produces disc depletion.
| Original language | English |
|---|---|
| Pages (from-to) | 392-393 |
| Number of pages | 2 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 5 |
| Issue number | S262 |
| DOIs | |
| State | Published - Aug 2009 |
| Externally published | Yes |
Keywords
- Binaries: mass loss
- Evolution
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