年轻超新星的高分辨率射电成像
天体物理学
2007-05-23 v2
摘要
通过使用 VLBI 可获得的高分辨率，为直接观察扩张的射电超新星与其周围介质的相互作用提供了独一无二的机会。我们在这里报告了对年轻超新星 SN 1979C、SN 1986J 和 SN 2001gd 的 VLBI 观测结果。
引用
@article{arxiv.astro-ph/0403273,
title = {High-resolution radio imaging of young supernovae},
author = {M. A. Perez-Torres and J. M. Marcaide and A. Alberdi and E. Ros and J. C. Guirado and L. Lara and F. Mantovani and C. J. Stockdale and K. W. Weiler and P. J. Diamond and S. D. Van Dyk and P. Lundqvist and N. Panagia and I. I. Shapiro and R. Sramek},
journal= {arXiv preprint arXiv:astro-ph/0403273},
year = {2007}
}
备注
8 pages, 3 figures. Uses svmult.cls. To appear in proceedings of IAU Colloquium 192 "Supernovae (10 years of SN 1993J)", April 2003, Valencia, Spain, eds. J. M. Marcaide and K. W. Weiler