Preprint
A Time-Dependent Spectral Analysis of γ Cassiopeiae
ArXiv.org
Cornell University
11/18/2024
DOI: 10.48550/arxiv.2411.11825
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.
Details
- Title: Subtitle
- A Time-Dependent Spectral Analysis of γ Cassiopeiae
- Creators
- Sean J Gunderson - Massachusetts Institute of TechnologyDavid P HuenemoerderJosé M TorrejónDustin K SwarmJoy S NicholsPragati PradhanRichard IgnaceHans Moritz Guenther - Massachusetts Institute of TechnologyA. M. T PollockNorbert S Schulz - Massachusetts Institute of Technology
- Resource Type
- Preprint
- Publication Details
- ArXiv.org
- DOI
- 10.48550/arxiv.2411.11825
- ISSN
- 2331-8422
- Publisher
- Cornell University; Ithaca, New York
- Language
- English
- Date posted
- 11/18/2024
- Academic Unit
- Physics and Astronomy
- Record Identifier
- 9984936604602771
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