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X-Ray Variability in M87: 1992-1998Beginning in 1995 June, we have obtained an observation of M 87 with the ROSAT High Resolution Imager (HRI) every 6 months. We present the measurements of X-ray intensity for the core and knot A through 1998 January. We find significant changes in both components. For the core, intensities measured in June 1995, December 1996, and December 1997 are roughly 30% higher than values obtained at three intervening times. For knot A, a secular decrease of approximately 15% is interrupted only by an intensity jump (3 sigma) in December 1997. Because the background used for subtraction is probably underestimated, we suspect the actual variation is somewhat greater than these values indicate.
Document ID
20000058174
Acquisition Source
Goddard Space Flight Center
Document Type
Other
Authors
Harris, D. E.
(Smithsonian Astrophysical Observatory Cambridge, MA United States)
Biretta, J. A.
(Space Telescope Science Inst. Baltimore, MD United States)
Junor, W.
(New Mexico Univ. Albuquerque, NM United States)
Date Acquired
September 7, 2013
Publication Date
January 1, 1998
Subject Category
Space Radiation
Funding Number(s)
CONTRACT_GRANT: NAG5-2957
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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