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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 7.

Spin phase–resolved NuSTAR spectroscopy of OAO 1657–415 for 16 phase bins. From top to bottom are the normalized intensity of the pulse profiles, absorption column density NH2 (in units of 1022 cm−2), covering fraction f, Fe Kα normalization (Fenorm; in photons cm−2 s−1), spectral index Γ, normalization of the power law (Γnorm; in photons keV−1 cm−2 s−1 at 1 keV), and folding energy (E fold; in keV). The corner plots of the third, seventh, and 13th phase bins, where the absorbing column density is low, high, and medium, respectively, are shown in Figure A5, A6, and A7.

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