تقرير
Chandra, NuSTAR, and Optical Observations of the Cataclysmic Variables IGR J17528-2022 and IGR J20063+3641
| العنوان: | Chandra, NuSTAR, and Optical Observations of the Cataclysmic Variables IGR J17528-2022 and IGR J20063+3641 |
|---|---|
| المؤلفون: | Hare, Jeremy, Halpern, Jules P., Tomsick, John A., Thorstensen, John R., Bodaghee, Arash, Clavel, Maica, Krivonos, Roman, Mori, Kaya |
| سنة النشر: | 2021 |
| المجموعة: | Astrophysics |
| مصطلحات موضوعية: | Astrophysics - High Energy Astrophysical Phenomena |
| الوصف: | 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$\alpha$ 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$\pm0.01$ s, which we attribute to the white dwarf spin period. Additional MDM spectroscopy of the source has also allowed for a clear determination of the orbital period at 0.731$\pm0.015$ d. The X-ray spectrum of this source is also well fit by an absorbed partially covered thermal bremsstrahlung model. The X-ray spectrum, spin periodicity, and orbital periodicity allow this source to be further classified as an intermediate polar. Comment: Accepted for publication in the Astrophysical Journal |
| نوع الوثيقة: | Working Paper |
| DOI: | 10.3847/1538-4357/abfa96 |
| الوصول الحر: | http://arxiv.org/abs/2104.10503Test |
| رقم الانضمام: | edsarx.2104.10503 |
| قاعدة البيانات: | arXiv |
| DOI: | 10.3847/1538-4357/abfa96 |
|---|