矮晕星外变动的光度曲线
天体物理学
2007-05-23 v1
摘要
我们将 AAVSO 和 VSS/RASNZ 的光度曲线与 Extreme Ultraviolet Explorer EUV 光度曲线组合，用于约束矮晕星外变动的本质。通过观察到的光学-EUV 时间延迟为 0.75-1.5 天，我们显示矮晕星不稳定加热波的传播速度约为 3 km/s。
引用
@article{arxiv.astro-ph/0011347,
title = {Optical and EUV Light Curves of Dwarf Nova Outbursts},
author = {Christopher W. Mauche and Janet A. Mattei and Frank M. Bateson},
journal= {arXiv preprint arXiv:astro-ph/0011347},
year = {2007}
}
备注
5 pages including 2 tables and 11 encapsulated postscript figures; LaTeX format, uses newpasp.sty; submitted for inclusion in the proceedings of "Evolution of Binary and Multiple Star Systems."