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The white dwarf initial-final mass relationship is shown for the 18 white dwarfs spectroscopically fit
The white dwarf initial-final mass relationship is shown for the 18 white dwarfs spectroscopically fit in this work (circles) and all previous constraints (triangles). Also shown are several semi-empirical and theoretical relations discussed in the Kalirai et al. paper. Bottom - A closer look at those white dwarfs that form the tight sequence with initial mass between 2.8 - 3.4 solar masses.
Créditos:International Gemini Observatory/NOIRLab/NSF/AURA
About the Image
Id: | geminiann05001c |
Tipo: | Chart |
Release date: | 27 de Enero de 2005 a las 05:00 |
Related announcements: | geminiann05001 |
Size: | 500 x 500 px |
Sobre el Objeto
Categoría: | Illustrations |