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Further observations of the burst source MXB 1728-34MXB 1728-34 has been observed by the SAS 3 observatory on eight occasions. It was bursting 95-100 per cent of the time, with burst intervals from 4 to 8 hr. The burst intervals were not correlated with the burst intensities. Seven relatively hard bursts occurring in July 1976 were all observed at energies up to about 30 keV. Following each of these bursts, enhanced X-ray emission was observed for several minutes, with a much softer spectrum than that of the bursts themselves. No periodic pulsations were observed from the associated steady source.
Document ID
19770049498
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
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.
(MIT Cambridge, Mass., United States)
Date Acquired
August 8, 2013
Publication Date
May 1, 1977
Publication Information
Publication: Royal Astronomical Society
Subject Category
Astrophysics
Accession Number
77A32350
Funding Number(s)
CONTRACT_GRANT: NAS5-11450
Distribution Limits
Public
Copyright
Other

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