河外经典新星M31N 2017-09a的不寻常爆发
太阳与恒星天体物理
2020-06-19 v1
摘要
M31N 2017-09a是一颗经典新星，在其初始爆发后约160天内被观测到，期间经历了若干次明亮的次级爆发。光变曲线以持续变化为特征，在日时间尺度上有至少0.5星等的偏离。爆发的下包络表明单一幂律可描述其下降速率。该爆发相对较长，其中，天。
引用
@article{arxiv.2006.10118,
title = {The Unusual Eruption of the Extragalactic Classical Nova M31N 2017-09a},
author = {Christopher Lloyd and Lewis M. Cook and Seiichiro Kiyota and Hanjie Tan and Di Hu and Wei Shi and Mi Zhang and Shenwei Zhang and Xiaowei Zhang and Jingyuan Zhao and Guoyou Sun and Xing Gao and David Boyd},
journal= {arXiv preprint arXiv:2006.10118},
year = {2020}
}
备注
8 pages, 3 figures