Project Details
Description
EO14042 THE LONG-AWAITED HAWC DISCOVERY OF TEV GAMMA-RAY EMISSION FROM THE EASTERN AND WESTERN LOBES OF W50 NEBULA POWERED BY THE MICROQUASAR SS433 WAS THE FIRST EVIDENCE THAT ACCRETING X-RAY BINARIES CAN EFFICIENTLY ACCELERATE PARTICLES TO TEV-PE
| Status | Finished |
|---|---|
| Effective start/end date | 1/1/22 → 12/31/22 |
Funding
- Goddard Space Flight Center: US$86,775.00
ASJC Scopus Subject Areas
- Astronomy and Astrophysics
- Radiation
- Physics and Astronomy(all)
- Aerospace Engineering
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