As the dense molecular cloud that was the precursor of our Solar System was collapsing to form a protosun and the surrounding solar-nebula accretion disk, infalling interstellar grains were heated much more effectively by radiation from the forming protosun than by radiation from the disk's accretio
โฆ LIBER โฆ
Clumping of Interstellar grains during formation of the primitive solar nebula
โ Scribed by A.G.W. Cameron
- Publisher
- Elsevier Science
- Year
- 1975
- Tongue
- English
- Weight
- 441 KB
- Volume
- 24
- Category
- Article
- ISSN
- 0019-1035
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