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19 April 2024
 
  » arxiv » astro-ph/0506186

 Article overview


Infrared Echoes near the Supernova Remnant Cassiopeia A
O. Krause ; G. H. Rieke ; S. M. Birkmann ; E. Le Floc’h ; K. D. Gordon ; E. Egami ; J. Bieging ; J. P. Hughes ; E. T. Young ; J. L. Hinz ; S. P. Quanz ; D. C. Hines ;
Date 8 Jun 2005
Subject astro-ph
AbstractTwo images of Cassiopeia A obtained at 24 micrometer with the Spitzer Space Telescope over a one year time interval show moving structures outside the shell of the supernova remnant to a distance of more than 20 arcmin. Individual features exhibit apparent motions of 10 to 20 arcsec per year, independently confirmed by near-infrared observations. The observed tangential velocities are at roughly the speed of light. It is likely that the moving structures are infrared echoes, in which interstellar dust is heated by the explosion and by flares from the compact object near the center of the remnant.
Source arXiv, astro-ph/0506186
Other source [GID 355916] pmid15947181
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