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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 11.

The coherence timescale τ of the column density time series is represented in kiloseconds at the top, and the color map shows the standard deviation δ N H for different clump sizes and masses. The values of orbital separation, orbital inclination, eccentricity, longitude of periastron, and periastron angle are taken from Jenke et al. (2012), and the orbital phase of the pulsar is 0.25.

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