Two component model best fits
Results showing that a two component model best fits the emission detected near Zeta Leporis. A single 2-4 AU annulus does not provide the correct FWHM while a lone 8-10 AU ring exhibits too much extended emission.
Credit:International Gemini Observatory/NOIRLab/NSF/AURA
About the Image
| Id: | geminiann07001b |
| Type: | Chart |
| Release date: | Jan. 19, 2007, 2:07 p.m. |
| Related announcements: | geminiann07001 |
| Size: | 500 x 316 px |
About the Object
| Category: | Illustrations |
