'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

Project: Research project

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

StatusFinished
Effective start/end date7/23/081/13/10

Funding

  • National Aeronautics and Space Administration: $26,400.00

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