Published January 1988
| Version v1
Journal article
Evolution of dust condensations in a protoplanetary disk
Description
After the dust sedimentation in a circumsolar protoplanetary disk and gravitational instability in the dust subdisk, the dust condensations are formed. The relations between the radius, mass, density and momentum of rotating condensations are investigated. The time of their growth and transformation into solid bodies is estimated. The biggest of them can evolve into protoplanets
Additional details
Additional titles
- Original title (Russian)
- Эволюция пылевых сгущений в допланетном диске
Publishing Information
- Journal Title
- Astron. Zh.
- Journal Volume
- 65
- Journal Issue
- 1
- Series
- Astron. Zh.
- Journal Page Range
- 58-72
- ISSN
- 0004-6299
- CODEN
- ASZHA
INIS
- Country of Publication
- Russian Federation
- Country of Input or Organization
- USSR
- INIS RN
- 19094332
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANGULAR MOMENTUM; CONDENSATES; CORRELATIONS; COSMIC DUST; MASS; PROTOPLANETS; ROTATION; SIZE; SOLAR NEBULA; SOLAR SYSTEM EVOLUTION
- Descriptors DEC
- DUSTS; NEBULAE