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A Time-Dependent Spectral Analysis of γ Cassiopeiae
Preprint   Open access

A Time-Dependent Spectral Analysis of γ Cassiopeiae

Sean J Gunderson, David P Huenemoerder, José M Torrejón, Dustin K Swarm, Joy S Nichols, Pragati Pradhan, Richard Ignace, Hans Moritz Guenther, A. M. T Pollock and Norbert S Schulz
ArXiv.org
Cornell University
11/18/2024
DOI: 10.48550/arxiv.2411.11825
url
https://doi.org/10.48550/arxiv.2411.11825View
Preprint (Author's original)This preprint has not been evaluated by subject experts through peer review. Preprints may undergo extensive changes and/or become peer-reviewed journal articles. Open Access

Abstract

We investigated the temporal and spectral features of \gamma Cassiopeiae's X-ray emission within the context of the white dwarf accretion hypothesis. We find that the variabilities present in the X-ray data show two different signals, one primarily due to absorption and the other due to flickering like in non-magnetic cataclysmic variables. We then use this two-component insight to investigate previously un-reported simultaneous XMM and NuSTAR data. The model fitting results find white dwarf properties consistent with optical studies alongside a significant secondary, thermal source. We propose a secondary shock between the Be decretion disk and white dwarf accretion disk as the source. Finally, we analyzed a unique, low-count rate event of the XMM light curve as potential evidence for the white dwarf encountering Be decretion disk structures.
Physics - High Energy Astrophysical Phenomena Physics - Solar and Stellar Astrophysics

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