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19 April 2024
 
  » arxiv » astro-ph/9708262

 Article overview


Deceleration in the Expansion of SN1993J
J. M. Marcaide ; A. Alberdi ; E. Ros ; P. Diamond ; I. I. Shapiro ; J. C. Guirado ; D. L. Jones ; F. Mantovani ; M. A. Perez-Torres ; R. A. Preston ; R. T. Schilizzi ; R. A. Sramek ; C. Trigilio ; S.D. Van Dyk ; K. W. Weiler ; A. R. Whitney ;
Date 28 Aug 1997
Journal Astrophys.J. 486 (1997) L31
Subject astro-ph
AbstractA rarity among supernova, SN 1993J in M81 can be studied with high spatial resolution. Its radio power and distance permit VLBI observations to monitor the expansion of its angular structure. This radio structure was previously revealed to be shell-like and to be undergoing a self-similar expansion at a constant rate. From VLBI observations at the wavelengths of 3.6 and 6 cm in the period 6 to 42 months after explosion, we have discovered that the expansion is decelerating. Our measurement of this deceleration yields estimates of the density profiles of the supernova ejecta and circumstellar material in standard supernova explosion models.
Source arXiv, astro-ph/9708262
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