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Two Decades in the Life of EXO 2030+375EXO 2030+375, a 42-s accreting pulsar in a 46-day orbit around a Be star, has undergone a detected outburst at nearly every periastron passage since 1991. It has been monitored with BATSE, RXTE, and Fermi/GBM. We will present preliminary results of long-term monitoring, including a long-term frequency history, long-term pulsed flux measurements, and available long ]term optical/ir monitoring results.
Document ID
20120016334
Acquisition Source
Marshall Space Flight Center
Document Type
Conference Paper
Authors
Wilson-Hodge, Colleen A. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Jenke, Pete (Alabama Univ. Huntsville, AL, United States)
Finger, Mark (Universities Space Research Association Huntsville, AL, United States)
Camero-Arranz, Ascension (Universities Space Research Association United States)
Fabregat, Juan (Valencia Univ. Spain)
Reig, Pablo (Southampton Univ. United Kingdom)
Steele, Iain (Liverpool John Moores Univ. Liverpool, United Kingdom)
Date Acquired
August 26, 2013
Publication Date
July 11, 2011
Subject Category
Astronomy
Report/Patent Number
M11-0561
Meeting Information
Meeting: BeXRB 2011
Location: Valencia
Country: Spain
Start Date: July 11, 2011
End Date: July 14, 2011
Distribution Limits
Public
Copyright
Public Use Permitted.

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