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Australian rocket resultsCen X-3 was observed twice. A pulse profile and spectrum was obtained in the 2- to 10-keV band, but no soft flux was detected. Vela X-1 was observed to have a rapid flickering characteristic on time scales down to 0.25 sec and a hard spectrum. The source 3U 0614+09 was observed and found to have a softer spectrum (kT of about 4 keV) and an intensity comparable to that of earlier observations. The source eta Car was not detected at a level of 0.03 ph/sq cm/sec in the band from 0.2 to 1.5 keV, and the Large Magellanic Cloud was observed in the band from 0.5 to 1.5 keV at a level of about 0.1 ph/sq cm/sec. Two soft extended regions were observed in Gem-Mon and Eridanus.
Document ID
19750051481
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Garmire, G.
(California Institute of Technology Pasadena, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
January 1, 1975
Subject Category
Astronomy
Meeting Information
Meeting: International Conference on X-Rays in Space - Cosmic, Solar, and Auroral X-Rays, Calgary
Location: Alberta
Country: Canada
Start Date: August 14, 1974
End Date: August 21, 1974
Accession Number
75A35553
Funding Number(s)
CONTRACT_GRANT: NGR-05-002-284
CONTRACT_GRANT: NGL-05-002-207
Distribution Limits
Public
Copyright
Other

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