Imaging of the Vega Debris System Using JWST/MIRI
We present images of the Vega planetary debris disk obtained at 15.5, 23, and 25.5 μ m with the Mid-Infrared Instrument on JWST. The debris system is remarkably symmetric, smooth, and centered accurately on the star. There is a broad Kuiper-belt-analog ring at ∼80–170 au that coincides with the plan...
Furkejuvvon:
| Váldodahkkit: | , , , , , , , , |
|---|---|
| Materiálatiipa: | Artigo |
| Giella: | Inglês |
| Almmustuhtton: |
IOP Publishing
2024-01-01
|
| Ráidu: | The Astrophysical Journal |
| Fáttát: | |
| Liŋkkat: | https://doi.org/10.3847/1538-4357/ad8cde |
| Fáddágilkorat: |
Eai fáddágilkorat, Lasit vuosttaš fáddágilkora!
|