Detection of X-ray periodicity from a new eclipsing polar candidate XGPS-I J183251-100106

C. Y. Hui; K. A. Seo; C. P. Hu; L. C.C. Lin; Y. Chou

doi:10.1088/0004-637X/759/2/109

Detection of X-ray periodicity from a new eclipsing polar candidate XGPS-I J183251-100106

C. Y. Hui
, K. A. Seo
, C. P. Hu
, L. C.C. Lin
, Y. Chou

天文研究所

研究成果: 雜誌貢獻 › 期刊論文 › 同行評審

5 引文斯高帕斯（Scopus）

摘要

We report the results from a detailed analysis of an archival XMM-Newton observation of the X-ray source XGPS-I J183251-100106, which has been suggested as a promising magnetic cataclysmic variable (CV) candidate based on its optical properties. A single periodic signal of 1.5 hr is detected from all EPIC instruments on board XMM-Newton. The phase-averaged X-ray spectrum can be well modeled with a thermal bremsstrahlung temperature of kT 50 keV. Both the X-ray spectral and temporal behavior of this system suggest that it is an eclipsing CV of the AM Herculis (or polar) type.

原文	???core.languages.en_GB???
文章編號	109
期刊	Astrophysical Journal
卷	759
發行號	2
DOIs	https://doi.org/10.1088/0004-637X/759/2/109
出版狀態	已出版 - 10 11月 2012

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10.1088/0004-637X/759/2/109

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title = "Detection of X-ray periodicity from a new eclipsing polar candidate XGPS-I J183251-100106",

abstract = "We report the results from a detailed analysis of an archival XMM-Newton observation of the X-ray source XGPS-I J183251-100106, which has been suggested as a promising magnetic cataclysmic variable (CV) candidate based on its optical properties. A single periodic signal of 1.5 hr is detected from all EPIC instruments on board XMM-Newton. The phase-averaged X-ray spectrum can be well modeled with a thermal bremsstrahlung temperature of kT 50 keV. Both the X-ray spectral and temporal behavior of this system suggest that it is an eclipsing CV of the AM Herculis (or polar) type.",

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T1 - Detection of X-ray periodicity from a new eclipsing polar candidate XGPS-I J183251-100106

AU - Hui, C. Y.

AU - Seo, K. A.

AU - Hu, C. P.

AU - Lin, L. C.C.

AU - Chou, Y.

PY - 2012/11/10

Y1 - 2012/11/10

N2 - We report the results from a detailed analysis of an archival XMM-Newton observation of the X-ray source XGPS-I J183251-100106, which has been suggested as a promising magnetic cataclysmic variable (CV) candidate based on its optical properties. A single periodic signal of 1.5 hr is detected from all EPIC instruments on board XMM-Newton. The phase-averaged X-ray spectrum can be well modeled with a thermal bremsstrahlung temperature of kT 50 keV. Both the X-ray spectral and temporal behavior of this system suggest that it is an eclipsing CV of the AM Herculis (or polar) type.

AB - We report the results from a detailed analysis of an archival XMM-Newton observation of the X-ray source XGPS-I J183251-100106, which has been suggested as a promising magnetic cataclysmic variable (CV) candidate based on its optical properties. A single periodic signal of 1.5 hr is detected from all EPIC instruments on board XMM-Newton. The phase-averaged X-ray spectrum can be well modeled with a thermal bremsstrahlung temperature of kT 50 keV. Both the X-ray spectral and temporal behavior of this system suggest that it is an eclipsing CV of the AM Herculis (or polar) type.

KW - X-rays: stars

KW - stars: individual (XGPS-I J183251-100106, 2XMM J183251.4-100106)

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ER -

Detection of X-ray periodicity from a new eclipsing polar candidate XGPS-I J183251-100106

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