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C. Caldwell, D. A. Moffett (Furman University), E. Reynoso (IAFE, Buenos Aires, Argentina)
We present results that trace the dynamics of two historical remnants, SN1006 and SN1572 (Tycho), for the past two decades. 21-cm radio images of each remnant were recorded during two previous epochs: 1983-1984 and 1991-1994. We obtained third-epoch images of both remnants from 2001 to 2003. After a direct comparison of images from these three epochs, we found the mean radio expansion rate of Tycho now agrees with a previous X-ray expansion study, and for the first time, we have measured the expansion rate over the entire rim of SN1006.
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Bulletin of the American Astronomical Society, 35#5
© 2003. The American Astronomical Soceity.