DOI:
10.1126/science.270.5241.1475
Authors:
MARCAIDE, JM; ALBERDI, A; ROS, E; DIAMOND, P; SHAPIRO, II; GUIRADO, JC; JONES, DL; KRICHBAUM, TP; MANTOVANI, F; PRESTON, RA; RIUS, A; SCHILIZZI, RT; TRIGILIO, C; WHITNEY, AR; WITZEL, A
Abstract:
A sequence of images from very long baseline interferometry shows that the young radio supernova SN 1993J is expanding with circular symmetry. However, the circularly symmetric images show emission asymmetries. A scenario in which freely expanding supernova ejecta shock mostly isotropic circumstellar material is strongly favored. The sequence of images constitutes the first ''movie'' of a radio supernova.
URL:
https://ui.adsabs.harvard.edu/#abs/1995Sci...270.1475M/abstract