A Dust-Scattering Model for M1-92: A Revised Estimate of the Mass Distribution and Inclination
Preplanetary nebulae (PPNe) are formed from mass-ejecting late-stage AGB stars. Much of the light from the star gets scattered or absorbed by dust particles, giving rise to the observed reflection nebula seen at visible and near-IR wavelengths. Precursors to planetary nebulae (PNe), PPNe generally h...
| الحاوية / القاعدة: | Galaxies |
|---|---|
| المؤلفون الرئيسيون: | , , |
| التنسيق: | مقال |
| اللغة: | الإنجليزية |
| منشور في: |
MDPI AG
2024-08-01
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| الموضوعات: | |
| الوصول للمادة أونلاين: | https://www.mdpi.com/2075-4434/12/4/44 |