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相关论文: Confirmation of IGR J01363+6610 as a Be X-ray bina…

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We present new results from INTEGRAL and Swift observations of the hitherto poorly studied and unidentified X-ray source XTE J1906+090. A bright hard X-ray outburst (luminosity of $\sim$10$^{36}$ erg s$^{-1}$ above 20 keV) has been…

高能天体物理现象 · 物理学 2023-05-24 V. Sguera , L. Sidoli , A. J. Bird , N. La Palombara

The X-ray pulsar SAX J0635+0533 was repeatedly observed with the XMM-Newton satellite in 2003-2004. The precise localization provided by these observations confirms the association of SAX J0635+0533 with a Be star. The source was found, for…

高能天体物理现象 · 物理学 2015-05-13 Sandro Mereghetti , Nicola La Palombara

AX J1749.1-2733 is an unclassified transient X-ray source discovered during surveys by ASCA in 1993-1999. A multi-wavelength study in NIR, optical, X-rays and hard X-rays is undertaken in order to determine its nature. AX J1749.1-2733 is a…

天体物理学 · 物理学 2008-09-08 J. A. Zurita Heras , S. Chaty

We report on the results of X-ray observations (XMM-Newton, INTEGRAL and Swift) of two hard X-ray sources, IGR J17503-2636 and IGR J17507-2647, whose nature is not fully elucidated in the literature. Three XMM-Newton observations covered…

高能天体物理现象 · 物理学 2024-11-27 L. Sidoli , V. Sguera , P. Esposito , R. Sathyaprakash , G. Ponti , S. Mondal , A. J. Bird

We report on the results of observations of hard X-ray sources in the Galactic plane with the Chandra X-ray Observatory. The hard X-ray IGR sources were discovered by the INTEGRAL satellite, and the goals of the Chandra observations are to…

天体物理学 · 物理学 2009-11-13 John A. Tomsick , Sylvain Chaty , Jerome Rodriguez , Roland Walter , Philip Kaaret

LSI +61 303 is one of the few X-ray binaries with Be star companion from which both radio and high-energy gamma-ray emission have been observed. We present XMM-Newton and INTEGRAL observations which reveal variability of the X-ray spectral…

天体物理学 · 物理学 2008-11-26 M. Chernyakova , A. Neronov , R. Walter

We report on the XMM-Newton observation of the Be/neutron star X-ray binary system RX J0146.9+6121, a long period (~ 23 m) pulsar in the NGC 663 open cluster. The X-ray luminosity decreased by a factor two compared to the last observation…

天体物理学 · 物理学 2009-11-11 Nicola La Palombara , Sandro Mereghetti

We observed 7 INTEGRAL sources with the Chandra X-ray Observatory to refine their localization to ~2 arcsec and to study their X-ray spectra. Two sources are inferred to have a Galactic origin: IGR J08390-4833 is most likely a magnetic…

天体物理学 · 物理学 2015-05-13 S. Sazonov , M. Revnivtsev , R. Burenin , E. Churazov , R. Sunyaev , W. R. Forman , S. S. Murray

The aim of this work is to characterize the counterpart to the INTEGRAL High Mass X-ray Binary candidate IGR J19294+1816 so as to establish its true nature. We obtained H band spectra of the selected counterpart acquired with the NICS…

高能天体物理现象 · 物理学 2018-02-28 J. J. Rodes-Roca , G. Bernabeu , A. Magazzù , J. M. Torrejón , E. Solano

IGR J01583+6713 is a new transient source discovered by the INTEGRAL/IBIS hard X-ray surveys. Optical observations suggested that it should be a high mass X-ray binary, but its nature is still unclear. We used the INTEGRAL/IBIS data to…

高能天体物理现象 · 物理学 2015-05-14 W. Wang

IGR J17091-3624 was discovered in 2003 April by INTEGRAL/IBIS during its Galactic Centre Deep Exposure programme. The source was initially detectable only in the 40--100 keV range, but after two days was also detected in the 15-40 keV…

We present the results of the XMM-Newton observations of five hard X-ray emitters: IGR J08262-3736, IGR J17354-3255, IGR J16328-4726, SAX J1818.6-1703, and IGR J17348-2045. The first source is a confirmed supergiant high mass X-ray binary,…

高能天体物理现象 · 物理学 2015-06-05 E. Bozzo , L. Pavan , C. Ferrigno , M. Falanga , S. Campana , S. Paltani , L. Stella , R. Walter

We report the first broad-band (0.5-150 keV) simultaneous X-ray observations of the very faint X-ray transient IGRJ17285-2922/XTEJ1728-295 performed with XMM-Newton and INTEGRAL satellites during its last outburst, started on 2010, August…

高能天体物理现象 · 物理学 2015-05-27 L. Sidoli , A. Paizis , S. Mereghetti , D. Gotz , M. Del Santo

We report on the discovery of X-ray pulsations in the Be/X-ray binary IGR J21343+4738 during an XMM-Newton observation. We obtained a barycentric corrected pulse period of 320.35+-0.06 seconds. The pulse profile displays a peak at low…

高能天体物理现象 · 物理学 2015-06-19 P. Reig , A. Zezas

We report on 0.3-10 keV observations with the Chandra X-ray Observatory of eight hard X-ray sources discovered within 8 degrees of the Galactic plane by the INTEGRAL satellite. The short (5 ks) Chandra observations of the IGR source fields…

IGR J18214-1318, a Galactic source discovered by the International Gamma-Ray Astrophysics Laboratory, is a high-mass X-ray binary (HMXB) with a supergiant O-type stellar donor. We report on the XMM-Newton and NuSTAR observations that were…

IGR J18219-1347 is a hard X-ray source discovered by INTEGRAL in 2010. We have analyzed the X-ray emission of this source exploiting the BAT survey data up to March 2012 and the XRT data that include also an observing campaign performed in…

高能天体物理现象 · 物理学 2015-06-16 V. La Parola , G. Cusumano , A. Segreto , A. D'Aì , N. Masetti , V. D'Elia

We report on the results of the multiwavelength campaign carried out after the discovery of the INTEGRAL transient IGR J17329-2731. The optical data collected with the SOAR telescope allowed us to identify the donor star in this system as a…

高能天体物理现象 · 物理学 2018-03-06 E. Bozzo , A. Bahramian , C. Ferrigno , A. Sanna , J. Strader , F. Lewis , D. M. Russell , T. di Salvo , L. Burderi , A. Riggio , A. Papitto , P. Gandhi , P. Romano

We studied the soft-X-ray emission of five hard-X sources: IGR J08262-3736, IGR J17354-3255, IGR J16328-4726, SAX J1818.6-1703 and IGR J17348-2045. These sources are: a confirmed supergiant high mass X-ray binary (IGR J08262-3736);…

高能天体物理现象 · 物理学 2013-03-20 L. Pavan , E. Bozzo , C. Ferrigno , M. Falanga , S. Campana , S. Paltani , L. Stella , R. Walter

We present the results of Chandra and XMM-Newton observations for six hard X-ray sources (IGR J12134-6015, IGR J18293-1213, IGR J18219-1347, IGR J17350-2045, IGR J18048-1455, XTE J1901+014) from the INTEGRAL all-sky survey. Based on these…

高能天体物理现象 · 物理学 2015-06-11 D. I. Karasev , A. A. Lutovinov , M. G. Revnivtsev , R. A. Krivonos
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