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SAS 3 observations of two X-ray transient events with precursorsSAS 3 has observed two unusual fast transient X-ray events from different sources, one lasting about 150 s and one, approximately 1500 s. Both events were preceded by precursor pulses which lasted a few seconds and which rose and fell in less than 0.4 s. The precursors were separated from the 'main' events by several seconds, during which no X-rays were detected. There are similarities between the two main events and X-ray bursts in both their temporal and spectral evolution. The spectra of the main events started out much softer than the spectra of the precursors, became harder as they approached maximum intensity, and softened as they decayed. In the 1500-s event, X-rays with energies greater than 10 keV were delayed by about 80 s compared with 1.5-6-keV X-rays. A blackbody fit to the spectral data of the main event of approximately 1500-s duration gives a maximum temperature of 29 million K and a radius for the emitting region of at least about 9 km (at a distance of 10 kpc); this is similar to the temperature and sizes found for several X-ray burst sources.
Document ID
19780048585
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hoffman, J. A.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lewin, W. H. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Doty, J.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Jernigan, J. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Haney, M.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Richardson, J. A.
(MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
April 15, 1978
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
78A32494
Funding Number(s)
CONTRACT_GRANT: NAS5-11450
Distribution Limits
Public
Copyright
Other

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