The radial velocities of the Balmer lines in WD 0931+444
The radial velocities of the Balmer lines in WD 0931+444. The bottom panel shows all of these data points phased with the best-fit period. The dotted line represents the best-fit model for a circular orbit with a period of 19.8 minutes.
Créditos:International Gemini Observatory/NOIRLab/NSF/AURA
About the Image
| Id: | geminiann14006c |
| Tipo: | Chart |
| Release date: | 16 de Junio de 2014 a las 14:06 |
| Related announcements: | geminiann14006 |
| Size: | 500 x 478 px |
Sobre el Objeto
| Nombre: | WD 0931+444 |
| Categoría: | Illustrations |
