Kühnel, M.Kretschmar, P.Nespoli, E.Okazaki, A.Schoenherr, G.Wilson-Hodge, C.Falkner, S.Brand, T.Anders, F.Schwarm, F.Kreykenbohm, I.Mueller, S.Pottschmidt, KatjaFuerst, F.Grinberg, V.Wilms, J.2023-09-062023-09-062015-03-16Kühnel, Matthias, Peter Kretschmar, Elisa Nespoli, Atsuo Okazaki, Gabriele Schoenherr, Colleen Wilson-Hodge, Sebastian Falkner, et al. “The Be X-Ray Binary Outburst Zoo II.” In Proceedings of 10th INTEGRAL Workshop: A Synergistic View of the High-Energy Sky — PoS(Integral2014), 228:078. SISSA Medialab, 2015. https://doi.org/10.22323/1.228.0078.https://doi.org/10.22323/1.228.0078http://hdl.handle.net/11603/2956610th INTEGRAL Workshop: "A Synergistic View of the High Energy Sky" - Integral2014, 15-19 September 2014, Annapolis, MD, USAWe 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+37510 pagesen-USThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.Public Domain Mark 1.0http://creativecommons.org/publicdomain/mark/1.0/The Be X-ray Binary Outburst Zoo IIText