夜间内耀变体变化的极端情况：S4 0954+65 案例
高能天体物理现象
2016-09-20 v1
摘要
我们展示了在夜间内时间尺度上对极端剧烈变化耀变体 S4 0954+65 的光学观测结果。该天体在几小时内显示出高达 100% 的流量变化。我们研究了光学波段间的时间延迟、颜色变化以及“rms-flux”关系，并基于现有的耀变体变化模型讨论了结果。
关键词
引用
@article{arxiv.1609.05303,
title = {The Extremes in Intra-Night Blazar Variability: The S4 0954+65 Case},
author = {Rumen Bachev and Anton Strigachev and Evgeni Semkov and Rosa Victoria Muñoz Dimitrova and Georgi Latev and Borislav Spassov and Blagovest Petrov},
journal= {arXiv preprint arXiv:1609.05303},
year = {2016}
}
备注
5 pages, accepted for publication in the special issue of Galaxies, "Blazars through Sharp Multi-wavelength Eyes", edited by J. L. G\'omez, A. P. Marscher, and S. G. Jorstad