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Be X-ray Binary Outburst Zoo II

Kühnel, Matthias and Kretschmar, Peter and Nespoli, Elisa and Okazaki, Atsuo T. and Schönherr, Gabriele and Wilson-Hodge, Colleen A. and Falkner, Sebastian and Brand, Thorsten and Anders, Friedrich and Schwarm, Fritz-Walter and Kreykenbohm, Ingo and Müller, Sebastian and Pottschmidt, Katja and Fürst, Felix and Grinberg, Victoria and Wilms, Jörn (2014) Be X-ray Binary Outburst Zoo II. In: 10th INTEGRAL Workshop: "A Synergistic View of the High Energy Sky" - Integral2014. Proceedings of Science. No.228. SISSA , Trieste, Italy, Art. No. 78. http://resolver.caltech.edu/CaltechAUTHORS:20180824-100034333

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Abstract

We have continued our recently started systematic study of Be X-ray binary (BeXRB) outbursts. Specifically, we are developing a catalogue of outbursts including their basic properties based on nearly all available X-ray all-sky-monitors. These properties are derived by fitting asymmetric Gaussians to the outburst lightcurves. This model describes most of the outbursts covered by our preliminary catalogue well; only 13% of all datasets show more complex outburst shapes. Analyzing the basic properties, we reveal a strong correlation between the outburst length and the reached peak flux. As an example, we discuss possible models describing the observed correlation in EXO 2030+375.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.22323/1.228.0078DOIBook Section
ORCID:
AuthorORCID
Pottschmidt, Katja0000-0002-4656-6881
Fürst, Felix0000-0003-0388-0560
Wilms, Jörn0000-0003-2065-5410
Additional Information:Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-ShareAlike. M. Kühnel acknowledges funding by the Bundesministerium für Wirtschaft und Technologie under Deutsches Zentrum für Luft- und Raumfahrt grant 50OR1113. The figures shown in this paper were created using the SLXfig module, which was developed by John E. Davis. We thank the organizers of the 10th Integral Workshop “A Synergistic View of the High Energy Sky” for the the useful discussions triggered by this interesting and well organized workshop.
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
Bundesministerium für Wirtschaft und Technologie (BMWi)UNSPECIFIED
Deutsches Zentrum für Luft- und Raumfahrt (DLR)50OR1113
Record Number:CaltechAUTHORS:20180824-100034333
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20180824-100034333
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:89144
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:24 Aug 2018 17:55
Last Modified:24 Aug 2018 17:55

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