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A 4.1 keV spectral feature in a type 1 X-ray burst from EXO 1747-214A spectral analysis of two type 1 bursts from EXO 1747-214 detected by Exosat is presented. During the rise of the strongest burst, the spectrum display a spectral feature which is well represented by an absorption line at 4.05 + or - 0.12 keV with an equivalent width of 570 + or - 87 eV and an upper limit to the line width at 800 eV. At all other times, the spectrum is well represented by that of a single blackbody. The observed line energy is compared with those observed in other burst and the possible origins of these lines are discussed.
Document ID
19890050218
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Magnier, Eugene
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Lewin, Walter H. G.
(Massachusetts Inst. of Tech. Cambridge, MA, United States)
Tan, Jianmin
(MIT Cambridge, MA, United States)
Van Paradijs, Jan
(Amsterdam, Universiteit; Nationaal Instituut voor Kernfysica en Hoge Energie Fysica, Netherlands)
Penninx, Wim
(MIT, Cambridge, MA; Nationaal Instituut voor Kernfysica en Hoge Energie Fysica Amsterdam, Netherlands)
Date Acquired
August 14, 2013
Publication Date
April 1, 1989
Publication Information
Publication: Royal Astronomical Society, Monthly Notices
Volume: 237
ISSN: 0035-8711
Subject Category
Astrophysics
Accession Number
89A37589
Funding Number(s)
CONTRACT_GRANT: NAG8-674
CONTRACT_GRANT: ZWO-782-371-019
CONTRACT_GRANT: NSG-7643
CONTRACT_GRANT: NAG8-571
Distribution Limits
Public
Copyright
Other

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