类星体黏滞危机
高能天体物理现象
2018-02-02 v1
摘要
近期对活动星系核极端变光现象的观测，已将标准黏滞吸积盘模型推至崩溃边缘。"极端再处理"机制中，一个不规则变化的中心准点源完全负责加热原本寒冷而被动的低黏滞吸积盘，或许是向前推进的最佳路径。
引用
@article{arxiv.1802.00408,
title = {Quasar Viscosity Crisis},
author = {Andy Lawrence},
journal= {arXiv preprint arXiv:1802.00408},
year = {2018}
}
备注
For consistency with Nature policy, the version posted here is the text as submitted to Nature Astronomy in November 2017. The final version is available at the DOI below, and differs slightly in wording. The final version can be posted in six months