Infrared Echoes near the Supernova Remnant Cassiopeia A
arXiv:astro-ph/0506186 · doi:10.1126/science.1112035
Abstract
Two 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.
arXiv commentTo be published in Science on June 10, 2005. 11 pages, 4 figures. Additional information available at http://www.spitzer.caltech.edu/Media/releases/ssc2005-14/index.shtml
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- Tycho Brahe's 1572 supernova as a standard type Ia explosion revealed from its light echo spectrum
- Dust and the type II-plateau supernova 2004et
- The Youngest Galactic Supernova Remnant: G1.9+0.3
- Supernova remnant energetics and magnetars: no evidence in favour of millisecond proto-neutron stars
- Constraints on the Progenitor of Cassiopeia A
- Scattered-Light Echoes from the Historical Galactic Supernovae Cassiopeia A and Tycho (SN 1572)
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- Direct Confirmation of the Asymmetry of the Cas A Supernova with Light Echoes
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- Central Compact Objects in Supernova Remnants
- Discovery of a 112 ms X-ray Pulsar in Puppis A: Further Evidence of Neutron Stars Weakly Magnetized at Birth
- Dust and the type II-Plateau supernova 2004dj
- Nuclear-Astrophysics Lessons from INTEGRAL
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- The Mid-Infrared Light Curve of Nearby Core-Collapse Supernova SN2011dh (PTF11eon)
- The Magnetic Field in Galaxies, Galaxy Clusters, and the InterGalactic Space
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- Observation of light echoes around very young stars
- A Search for Infrared Emission from Core-Collapse Supernovae at the Transitional Phase
- Probing Interstellar Dust with Infrared Echoes from the Cas A Supernova
- Searching for continuous gravitational waves from slowly spinning neutron stars with DECIGO, Big Bang Observer, Einstein Telescope and Cosmic Explorer
- JWST/MIRI detects the dusty SN1993J about 30 years after explosion
- Progress on multi-waveband observations of supernova remnants