狄拉西-布拉姆林 (DBL) IY UMa 在平静期的多普勒断层扫描
天体物理学
2007-05-23 v1
摘要
IY UMa 这一新发现的深层被掩埋的 SU UMa 系统在平静期的多普勒断层扫描揭示了来自 donor 向盘边缘冲击区域的属性。产生了非常强的亮斑，Kepler 盘发射在冲击区域被破坏或遮蔽。H-alpha、H-beta 和 He I 发射的差异性质将允许研究收敛流区域的物理参数。
引用
@article{arxiv.astro-ph/0009329,
title = {Doppler Tomography of Dwarf Nova IY UMa during Quiescence},
author = {Daniel J. Rolfe and Timothy M. C. Abbott and Carole A. Haswell},
journal= {arXiv preprint arXiv:astro-ph/0009329},
year = {2007}
}
备注
6 pages, 5 figures. To appear in Proceedings of Astro-Tomography Workshop, Brussels, July 2000, Eds. H. Boffin, D. Steeghs, Springer-Verlag Lecture Notes in Physics