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

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

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dc.contributor.author Martinez Nuñez, Silvia
dc.contributor.author Reig Torres, Pablo
dc.contributor.author Blay Serrano, Pedro Jose
dc.contributor.author Kretschmar, P.
dc.contributor.author Lund, N.
dc.contributor.author Reglero Velasco, Victor
dc.date.accessioned 2010-06-29T11:12:12Z
dc.date.available 2010-06-29T11:12:12Z
dc.date.issued 2003
dc.identifier.citation MARTINEZ NUÑEZ, Silvia ; Reig Torres, Pablo ; Blay Serrano, Pedro Jose ; Kretschmar, P. ; Lund, N. ; Reglero Velasco, Victor, 2003, JEM-X observations of the Be/X-ray binary EXO 2030+375, Astronomy and Astrophysics, vol. 411, no. 1, p. L411-L414 en
dc.identifier.uri http://hdl.handle.net/10550/14024
dc.description.abstract 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. en
dc.language.iso en en
dc.subject INTEGRAL ; JEM-X ; BeX stars ; HMXRBs ; EXO 2030+375 en
dc.title JEM-X observations of the Be/X-ray binary EXO 2030+375 en
dc.type journal article es_ES
dc.subject.unesco UNESCO::ASTRONOMÍA Y ASTROFÍSICA en
dc.subject.unesco UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia en
dc.identifier.doi 10.1051/0004-6361:20031205 en
dc.identifier.idgrec 003621 en
dc.type.hasVersion VoR es_ES
dc.identifier.url http://www.aanda.org/articles/aa/pdf/2003/43/aaINTEGRAL10.pdf en

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