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Clumpy Wind Studies and the Nondetection of a Cyclotron Line in OAO 1657–415

  • Authors: Pragati Pradhan, Carlo Ferrigno, Biswajit Paul, Enrico Bozzo, Ileyk El Mellah, David P. Huenemoerder, James F. Steiner, Victoria Grinberg, Felix Furst, Chandreyee Maitra, Patrizia Romano, Peter Kretschmar, Jamie Kennea, Deepto Chakrabarty

Pragati Pradhan et al 2023 The Astrophysical Journal 945 .

  • Provider: AAS Journals

Caption: Figure 3.

From top to bottom are the NuSTAR light curves (counts per second), HR with 20 time segments delimited by red vertical solid lines, absorption column density NH2 (in units of 1022 cm−2), covering fraction f, EW (in keV), normalization of the Fe Kα line Fenorm (in photons cm−2 s−1), spectral index Γ, folding energy E fold (in keV), normalization of the power law Γnorm (in photons keV−1 cm−2 s−1 at 1 keV), and absorbed flux in 3–70 keV (in 1 × 10−9 erg cm−2 s−1). The NH1 is frozen at the line-of-sight absorption of 1.8 × 1022 atoms cm−2. Note that not all parameters could be constrained in segment 10; therefore, no errors are plotted for this segment. The corner plots corresponding to some segments where the absorption values are medium, low, and high (1, 7, and 19) in these fits are shown in Figures A2A4.

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