Project Details
Description
'PROBING THE MAGNETIC CONFINEMENT OF THE WINDS OF OE STARS' The small group of Oe stars are usually considered as the hot analogs of the Be-type objects. A possible explanation for their equatorial outflow is that their stellar wind is magnetically channe
| Status | Finished |
|---|---|
| Effective start/end date | 7/23/08 → 1/13/10 |
Funding
- National Aeronautics and Space Administration: $26,400.00
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