Chandra, NuSTAR, and Optical Observations of the Cataclysmic Variables IGR J17528-2022 and IGR J20063+3641
Jeremy Hare, Jules P. Halpern, John A. Tomsick, John R. Thorstensen,, Arash Bodaghee, Maica Clavel, Roman Krivonos, and Kaya Mori

TL;DR
This study combines X-ray and optical observations to identify and classify two INTEGRAL sources, revealing one as a magnetic cataclysmic variable and the other as an intermediate polar, with detailed spectral and periodic analysis.
Contribution
It provides the first optical counterpart identification for IGR J17528-2022 and confirms the classification of IGR J20063+3641 as an intermediate polar through combined multi-wavelength observations.
Findings
IGR J17528-2022 is a strong magnetic CV candidate.
IGR J20063+3641 is an intermediate polar with a 172.46 s spin period.
Both sources' X-ray spectra are well fit by absorbed partially covered thermal bremsstrahlung models.
Abstract
We report on Chandra, NuSTAR, and MDM observations of two INTEGRAL sources, namely IGR J17528-2022 and IGR J20063+3641. IGR J17528-2022 is an unidentified INTEGRAL source, while IGR J20063+3641 was recently identified as a magnetic cataclysmic variable (mCV) by Halpern et al. (2018). The Chandra observation of IGR J17528-2022 has allowed us to locate the optical counterpart to the source and to obtain its optical spectrum, which shows a strong H emission line. The optical spectrum and flickering observed in the optical time-series photometry in combination with the X-ray spectrum, which is well fit by an absorbed partially covered thermal bremsstrahlung model, suggests that this source is a strong mCV candidate. The X-ray observations of IGR J20063+3641 reveal a clear modulation with a period of 172.46 s, which we attribute to the white dwarf spin period. Additional MDM…
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