类星体主序：极端天体的驯服
星系天体物理
2022-02-16 v1
摘要
过去几年见证了与类星体主序相关若干趋势的确认。类星体主序的概念相对新颖，其在类星体性质的观测分类与语境化方面的全部潜力尚待充分发掘。本文从极端天体的性质出发讨论主序的驱动因素。我们简要总结了对特定类星体类别（极端 Population B，以低 Eddington 比率辐射）吸积盘视角的约束进展，以及对宽线发射气体化学组成的推断，还有类星体主序上射电辐射本质的探讨。
引用
@article{arxiv.2111.04140,
title = {The Main Sequence of quasars: the taming of the extremes},
author = {P. Marziani and E. Bon and N. Bon and M. D'Onofrio and B. Punsly and M. Sniegowska and B. Czerny and S. Panda and M. L. Martinez Aldama and A. del Olmo and A. Deconto-Machado and C. A. Negrete and D. Dultzin and T. Buendia and K. Garnica},
journal= {arXiv preprint arXiv:2111.04140},
year = {2022}
}
备注
Paper presented at the XIII SCSLSA, to appear in Astronomische Nachrichten