THE THREE-DIMENSIONAL STRUCTURE OF CASSIOPEIA A
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DeLaney-2010-THE THREE-DIMENSIONA.pdf
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Author(s)
DeLaney, Tracey
Rudnick, Lawrence
Stage, M. D.
Smith, J. D.
Isensee, Karl
Rho, Jeonghee
Allen, Glenn E.
Gomez, Haley
Kozasa, Takashi
Reach, William T.
Date Issued
December 2010
Journal
Astrophysical Journal
Publisher
Institute of Physics/American Astronomical Society
Citation
DeLaney, Tracey, Lawrence Rudnick, M. D. Stage, J. D. Smith, Karl Isensee, Jeonghee Rho, Glenn E. Allen, et al. “THE THREE-DIMENSIONAL STRUCTURE OF CASSIOPEIA A.” The Astrophysical Journal 725, no. 2 (December 3, 2010): 2038–2058.
Version
Final published version
Abstract
We used the Spitzer Space Telescope's Infrared Spectrograph to map nearly the entire extent of Cassiopeia A between 5 and 40 μm. Using infrared and Chandra X-ray Doppler velocity measurements, along with the locations of optical ejecta beyond the forward shock, we constructed a three-dimensional model of the remnant. The structure of Cas A can be characterized into a spherical component, a tilted thick disk, and multiple ejecta jets/pistons and optical fast-moving knots all populating the thick disk plane. The Bright Ring in Cas A identifies the intersection between the thick plane/pistons and a roughly spherical reverse shock. The ejecta pistons indicate a radial velocity gradient in the explosion. Some ejecta pistons are bipolar with oppositely directed flows about the expansion center while some ejecta pistons show no such symmetry. Some ejecta pistons appear to maintain the integrity of the nuclear burning layers while others appear to have punched through the outer layers. The ejecta pistons indicate a radial velocity gradient in the explosion. In three dimensions, the Fe jet in the southeast occupies a "hole" in the Si-group emission and does not represent "overturning," as previously thought. Although interaction with the circumstellar medium affects the detailed appearance of the remnant and may affect the visibility of the southeast Fe jet, the bulk of the symmetries and asymmetries in Cas A are intrinsic to the explosion.
MIT Department
MIT Kavli Institute for Astrophysics and Space Research
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DOI of Published Version
https://doi.org/10.1088/0004-637x/725/2/2038
