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Journal article

JEM-X observations of the Be/X-ray binary EXO 2030+375

From

Astrophysics, National Space Institute, Technical University of Denmark1

National Space Institute, Technical University of Denmark2

We have used data from the Joint European Monitor (JEM-X) to perform an X-ray spectral and timing analysis of the 42-s transient pulsar EXO 2030+375 during an X-ray outburst. X-ray pulsations are clearly detected with an average pulse period of 41.66+/-0.05 s and an average pulse fraction of 60%. The profile of the energy spectrum did not change appreciably throughout the X-ray outburst, although the source shows a slightly softer spectrum during periastron passage in the energy range 9-25 keV.

The 5-25 keV X-ray luminosity changed by a factor of 2 throughout the observations, reaching a maximum value of 3x10(36) erg s(-1). These observations allowed us to verify the in-flight instrumental properties of the JEM-X Monitor.

Language: English
Publisher: EDP Sciences
Year: 2003
Pages: L411-L414
ISSN: 14320746 and 00046361
Types: Journal article
DOI: 10.1051/0004-6361:20031205
ORCIDs: Lund, Niels

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