Mass Spectrum and Velocity Dispersions During Planetesimals Accumulation - II - Fragmentation
arXiv:astro-ph/9304028 · doi:10.1006/icar.1993.1084
Abstract
Fragmentation of the planetesimals is found to play a role whose importance is greater than previously believed and depends on the average characteristic size of the primordial planetesimals but not on their mass distribution. In the small size range the mass spectrum is strongly modified with the formation of a small bodies tail but, on the other hand, the growth of the most massive objects is significantly slowed down. The formation of planetary embryos much more massive than the rest of the swarm is delayed; nevertheless the time-scale problem for the growth of the outer planets is not revived.
30 pp - plain TEX - Accepted to Icarus
Cited by in corpus (9)
- Accretion in the Early Kuiper Belt II. Fragmentation
- Accretion in the Early Kuiper Belt I. Coagulation and Velocity Evolution
- Relative velocities among accreting planetesimals in binary systems: the circumbinary case
- Collisional Cascades in Planetesimal Disks I. Stellar Flybys
- Planetary formation in the Gamma-Cephei system
- Planet formation in Alpha Centauri A revisited: not so accretion-friendly after all
- Planetesimal Accretion in Binary Systems: Could Planets Form Around Alpha Centauri B ?
- Planetesimal Accretion in Binary Systems: The Effects of Gas Dissipation
- Planetesimal Accretion in Binary Systems: Role of the Companion's Orbital Inclination