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AXAF/Chandra CapabilitiesI will show some examples of what can be done with AXAF/Chandra, whose mirror has a subarcsecond angular resolution and whose detectors include Charge-Coupled Devices (CCDs) and microchannel plates with available high spectral resolution gratings.
Document ID
19990072353
Acquisition Source
Marshall Space Flight Center
Document Type
Abstract
Authors
Markevitch, M.
(Smithsonian Astrophysical Observatory Cambridge, MA United States)
Date Acquired
August 19, 2013
Publication Date
January 1, 1999
Subject Category
Earth Resources And Remote Sensing
Meeting Information
Meeting: Heating and Acceleration in the Universe
Location: Tokyo
Country: Japan
Start Date: March 16, 1999
End Date: March 20, 1999
Sponsors: ASCA
Funding Number(s)
CONTRACT_GRANT: NAS-39073
Distribution Limits
Public
Copyright
Other

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