碰撞的稀薄前行星子的角动量
地球与行星天体物理
2014-12-30 v1
摘要
形成小天体双星所需的稀薄前行星子的角动量可以通过前行星子的碰撞获得。包括海王星外双星在内的海王星外天体，可能由收缩的稀薄前行星子形成。
引用
@article{arxiv.1412.8445,
title = {Angular momenta of collided rarefied preplanetesimals},
author = {Sergei I. Ipatov},
journal= {arXiv preprint arXiv:1412.8445},
year = {2014}
}
备注
4 pages. Proc. IAU Symp. No. 293 "Formation, detection, and characterization of extrasolar habitable planets", ed. by Nader Haghighipour, Proceedings of the International Astronomical Union, vol. 8, Symposium S293, Cambridge University Press. pp. 285-288. (2014)