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相关论文: Suzaku X-Ray Study of an Anomalous Source XSS J122…

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XSS J12270-4859 (J12270) is an enigmatic source of unknown nature. Previous studies revealed that the source has unusual X-ray temporal characteristics, including repetitive short-term flares followed by spectral hardening, non-periodic…

高能天体物理现象 · 物理学 2015-05-28 Kei Saitou , Masahiro Tsujimoto , Ken Ebisawa , Manabu Ishida , Koji Mukai , Takahiro Nagayama , Shogo Nishiyama , Poshak Gandhi

We report on the first Suzaku observation of IGR J16318-4848, the most extreme example of a new group of highly absorbed X-ray binaries that have recently been discovered by the International Gamma-Ray Astrophysics Laboratory INTEGRAL. The…

高能天体物理现象 · 物理学 2015-05-14 L. Barragán , J. Wilms , K. Pottschmidt , M. A. Nowak , I. Kreykenbohm , R. Walter , J. A. Tomsick

With the Suzaku satellite, we observed an unidentified TeV gamma-ray source HESS J1741$-$302 and its surroundings. No diffuse or point-like X-ray sources are detected from the bright southern emission peak of HESS J1741$-$302. From its…

高能天体物理现象 · 物理学 2015-05-28 Hideki Uchiyama , Katsuji Koyama , Hironori Matsumoto , Omar Tibolla , Sarah Kaufmann , Stefan Wagner

The anomalous X-ray pulsar 4U 0142+61 was observed with Suzaku on 2007 August 15 for a net exposure of -100 ks, and was detected in a 0.4 to ~70 keV energy band. The intrinsic pulse period was determined as 8.68878 \pm 0.00005 s, in…

Suzaku TOO observation of the anomalous X-ray pulsar CXOU J164710.2-455216 was performed on 2006 September 23--24 for a net exposure of 38.8 ks. During the observation, the XIS was operated in 1/8 window option to achieve a time resolution…

Suzaku observations are presented for the high-mass X-ray binaries IGR J16207-5129 and IGR J17391-3021 (=XTE J1739-302). For IGR J16207-5129, we provide the first X-ray broadband (0.5--60 keV) spectrum from which we confirm a large…

高能天体物理现象 · 物理学 2015-06-03 A. Bodaghee , J. A. Tomsick , J. Rodriguez , S. Chaty , K. Pottschmidt , R. Walter , P. Romano

We report on a 250 ks long X-ray observation of the supergiant fast X-ray transient (SFXT) IGR J16479-4514 performed with Suzaku in 2012 February. About 80% of the short orbital period (Porb=3.32 days) was covered as continuously as…

高能天体物理现象 · 物理学 2015-06-12 L. Sidoli , P. Esposito , V. Sguera , A. Bodaghee , J. A. Tomsick , K. Pottschmidt , J. Rodriguez , P. Romano , J. Wilms

The Galactic black-hole binary GRO J1655$-$40 was observed with Suzaku on 2005 September 22--23, for a net exposure of 35 ks with the X-ray Imaging Spectrometer (XIS) and 20 ks with the Hard X-ray Detector (HXD). The source was detected…

The nature of the hard X-ray source XSSJ12270-4859 is still unclear though it was claimed to be a magnetic Cataclysmic Variable. We here present a broad-band X-ray and gamma ray study based on a recent XMM-Newton observation and archival…

高能天体物理现象 · 物理学 2015-05-18 D. de Martino , M. Falanga , J. -M. Bonnet-Bidaud , T. Belloni , M. Mouchet , N. Masetti , I. Andruchow , S. A. Cellone , K. Mukai , G. Matt

SAX J1748.2$-$2808 is a unique X-ray object with a flat spectrum and strong emission lines at 6.4--7.0 keV. The Suzaku satellite resolved the emission lines into 3 K-shell lines from neutral and highly ionized irons. A clear coherent…

天体物理学 · 物理学 2015-05-13 Masayoshi Nobukawa , Katsuji Koyama , Hironori Matsumoto , Takeshi Go Tsuru

We report a serendipitous detection of an intense X-ray flare from the Tycho reference source HD 161084 during a Suzaku observation of the Galactic Center region for 20 ks. The X-ray Imaging Spectrometer (XIS) recorded a flare from this…

The X-ray source XSS J12270-4859 has been first suggested to be a magnetic cataclysmic variable of Intermediate Polar type on the basis of its optical spectrum and a possible 860 s X-ray periodicity. However further X-ray observations by…

空间物理 · 物理学 2012-02-14 J. M. Bonnet-Bidaud , D. de Martino , M. Mouchet , M. Falanga , T. Belloni , N. Masetti , K. Mukai , G. Matt

Five on-plane regions within +/- 0.8deg of the Galactic center were observed with the Hard X-ray Detector (HXD) and the X-ray Imaging Spectrometer (XIS) onboard Suzaku. From all regions, significant hard X-ray emission was detected with…

In this paper we study the timing and spectral properties of Be/X-ray binary pulsar EXO 2030+375 using a $Suzaku$ observation on 2012 May 23, during a less intense Type I outburst. Pulsations were clearly detected in the X-ray light curves…

太阳与恒星天体物理 · 物理学 2015-06-23 Sachindra Naik , Gaurava K. Jaisawal

In October 2007 a hard X-ray burst was detected by the INTEGRAL satellite from a direction consistent with the position of AX J1818.8-1559, an X-ray source at low Galactic latitude discovered with the ASCA satellite in 1996-1999. The short…

高能天体物理现象 · 物理学 2015-06-11 S. Mereghetti , P. Esposito , A. Tiengo , D. Gotz , G. L. Israel , A. De Luca

The eclipsing low-mass X-ray binary AX J1745.6-2901 was observed with Suzaku in its outburst phase. Combining the Chandra observation made 1.5 month earlier than Suzaku, we determined the orbital period to be 30063.76+/-0.14 s. We found…

We report here on the longest deep X-ray observation of a SFXT outside outburst, with an average luminosity level of 1E33 erg/s (assuming 3 kpc distance). This observation was performed with Suzaku in December 2009 and was targeted on…

高能天体物理现象 · 物理学 2015-05-19 L. Sidoli , P. Esposito , L. Ducci

We present the results from analyses of Suzaku observations of the supergiant X-ray binaries IGR J16207-5129 and IGR J17391-3021. For IGR J16207-5129, we provide the first broadband (0.5--60 keV) spectrum from which we confirm a large…

高能天体物理现象 · 物理学 2010-12-16 A. Bodaghee , J. A. Tomsick , J. Rodriguez , S. Chaty , K. Pottschmidt , R. Walter , P. Romano

We report the timing and broad-band spectral properties of the Be transient high mass X-ray binary pulsar GRO J1008-57 using a Suzaku observation in the declining phase of its 2007 November-December outburst. Pulsations with a period of…

太阳与恒星天体物理 · 物理学 2011-05-17 Sachindra Naik , Biswajit Paul , Chetan Kachhara , Santosh V. Vadawale

The bright X-ray source, 2XMMi J180438.7-145647 is fortunate to have long baseline observations in INTEGRAL that compliment observations taken by other missions. Optical spectroscopy of this object has suggested a distance of ~7 kpc and an…

高能天体物理现象 · 物理学 2015-05-30 Matthew J. Middleton , Edward M. Cackett , Craig Shaw , Gavin Ramsay , Timothy P. Roberts , Peter J. Wheatley
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