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X-ray imaging - Supernova remnantsConsideration is given to imaging observations of supernova remnants (SNRs) obtained during the first year of the Einstein Observatory's operation. Inferences are drawn regarding models for stellar explosions, remnant evolution, neutron star formation and the interstellar medium. Because the X-ray emission traces the expanding shock boundary and dominates the radiative energy losses of an SNR over much of its lifetime, it can provide data on the possible collapsed remnants of the explosion, such as neutron stars and/or black holes. X-ray emission also allows a supernova shock to be used as a probe of interstellar medium structure. The imaging instrument aboard the Einstein satellite has been used to observe over 30 known Galactic remnants, and a similar number of objects in other galaxies, in the 0.15-4.5 keV band.
Document ID
19820049944
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Helfand, D. J.
(Columbia University New York, NY, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1981
Subject Category
Astrophysics
Meeting Information
Meeting: In: X-ray astronomy with the Einstein satellite
Location: Cambridge, MA
Start Date: January 28, 1980
End Date: January 30, 1980
Accession Number
82A33479
Funding Number(s)
CONTRACT_GRANT: NAS8-30753
Distribution Limits
Public
Copyright
Other

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