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We aim at characterizing a sample of 9 new hard X-ray selected Cataclysmic Variable (CVs), to unambiguously identify them as magnetic systems of the Intermediate Polar (IP) type. We performed timing and spectral analysis by using X-ray, and…

High Energy Astrophysical Phenomena · Physics 2015-06-04 F. Bernardini , D. de Martino , M. Falanga , K. Mukai , G. Matt , J. -M. Bonnet-Bidaud , N. Masetti , M. Mouchet

Chandra X-ray observations of the high redshift (z =1.532) radio-loud quasar 3C270.1 in 2008 February show the nucleus to have a power-law spectrum, Gamma = 1.66 +/- 0.08, typical of a radio-loud quasar, and a marginally-detected Fe Kalpha…

The broadband X-ray spectrum of the prototypical starburst galaxy M82 is very complex. At least three spectral components are required to fit the combined ROSAT and ASCA spectrum in the 0.1--10 keV range. The observed X-ray flux in this…

Astrophysics · Physics 2009-10-28 Edward C. Moran , Matthew D. Lehnert

The X-ray spectrum from a cool disk embedded in an ion supported torus is computed. The interaction of the hot ions with the disk increases the hard X-ray luminosity of the system}. A surface layer of the disk is heated by the protons from…

Astrophysics · Physics 2009-10-31 H. C. Spruit , F. Haardt

This work presents the broad-band time-averaged spectral analysis of neutron star low-mass X-ray binary, XTE J1710-281 by using the Suzaku archival data. The source was in a hard or an intermediate spectral state during this observation.…

High Energy Astrophysical Phenomena · Physics 2020-06-17 Prince Sharma , Rahul Sharma , Chetana Jain , Anjan Dutta

We present results of X-ray observations of the Coma cluster with multiple instruments over a broad energy band. Using the data from INTEGRAL, RXTE and ROSAT observatories, we find that the Coma spectrum in the 0.5-107 keV energy band can…

Astrophysics · Physics 2009-11-13 A. A. Lutovinov , A. Vikhlinin , E. M. Churazov , M. G. Revnivtsev , R. A. Sunyaev

We present for the first time orbital phase-resolved spectra of an intermediate polar (IP), EX Hya, together with the spin phase-resolved spectra during two different epochs using the X-ray Multi-Mirror Mission, European Photon Imaging…

High Energy Astrophysical Phenomena · Physics 2010-09-23 Y. Pekon , S. Balman

We present the analysis of five joint XMM-Newton/NuSTAR observations, 20 ks each and separated by 12 days, of the broad-line radio galaxy 3C 382. The data were obtained as part of a campaign performed in September-October 2016…

High resolution X-ray spectroscopy of the warm absorber in the nearby X-ray bright Seyfert 1 galaxy, Mrk 1040 is presented. The observations were carried out in the 2013-2014 timeframe using the Chandra High Energy Transmission Grating with…

High Energy Astrophysical Phenomena · Physics 2017-03-08 James Reeves , Valentina Braito , Ehud Behar , Travis Fischer , Steve Kraemer , Andrew Lobban , Emanuele Nardini , Delphine Porquet , Jane Turner

Unified X-ray spectral and timing studies of Cygnus X-1 in the low/hard and hard intermediate state were conducted in a model-independent manner, using broadband Suzaku data acquired on 25 occasions from 2005 to 2009 with a total exposure…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Shin'ya Yamada , Kazuo Makishima , Chris Done , Shunsuke Torii , Hirofumi Noda , Soki Sakurai

We present the broad band X-ray spectrum of Cyg X-1 in the low/hard state as observed by the instruments on board of BeppoSAX. The spectrum spans from 0.1 to 200 keV, allowing the total accretion luminosity to be observed, rather than…

Astrophysics · Physics 2009-10-31 T. Di Salvo , C. Done , P. T. Zycki , L. Burderi , N. R. Robba

We present detailed analyses of oxygen K absorption in the interstellar medium (ISM) using four high-resolution Chandra spectra towards the X-ray low-mass binary XTE J1817-330. The 11-25 A broadband is described with a simple absorption…

High Energy Astrophysical Phenomena · Physics 2015-06-15 E. Gatuzz , J. García , C. Mendoza , T. R. Kallman , M. Witthoeft , A. Lohfink , M. A. Bautista , P. Palmeri , P. Quinet

We present an analysis of spectrum and variability of the bright reddened narrow line Seyfert 1 galaxy Was~61 using 90 ks archival {\it XMM-Newton} data. The X-ray spectrum in 0.2-10 keV can be characterized by an absorbed power-law plus…

High Energy Astrophysical Phenomena · Physics 2016-03-11 Liming Dou , Ting-Gui Wang , Yanli Ai , Weimin Yuan , Hongyan Zhou , Xiao-Bo Dong

Attempts were made to construct a unified description of the spectra of ULX (Ultra Luminous X-ray source) objects, including their Power-Law (PL) state and Disk-like state. Among spectral models proposed to explain either state, the present…

High Energy Astrophysical Phenomena · Physics 2016-05-25 S. Kobayashi , K. Nakazawa , K. Makishima

We report on the results of spectral analysis of the dipping source XB 1254-690 observed by the BeppoSAX satellite. We find that the X-ray dips are not present during the BeppoSAX observation, in line with recent RXTE results. The broad…

Astrophysics · Physics 2009-10-31 R. Iaria , T. Di Salvo , L. Burderi , N. R. Robba

A 0.5-200 keV BeppoSAX spectrum of the non-pulsating high-mass X-ray binary 4U1700-37 is presented. The spectrum is well characterized by the standard accreting pulsar model of an absorbed power-law with a photon index of 1.07 +0.02 -0.03,…

Astrophysics · Physics 2007-05-23 A. P. Reynolds , A. Owens , L. Kaper , A. N. Parmar , A. Segreto

The source 4U 1702-429 (Ara X-1) is a low-mass X-ray binary system hosting a neutron star. Albeit the source is quite bright ( $\sim10^{37}$ erg s$^{-1}$) its broadband spectrum has never been studied. Neither dips nor eclipses have been…

High Energy Astrophysical Phenomena · Physics 2016-11-30 R. Iaria , T. Di Salvo , M. Del Santo , F. Pintore , A. Sanna , A. Papitto , L. Burderi , A. Riggio , A. F. Gambino , M. Matranga

We present four X-ray/gamma-ray spectra of Cyg X-1 observed in the hard ('low') state simultaneously by Ginga and GRO/OSSE on 1991 July 6. The 3-30 keV Ginga spectra are well represented by power laws with an energy spectral index of…

We report the identification of the ROSAT all-sky survey source 1RXS J154814.5-452845as new intermediate polar and present the results from follow-up optical and X-ray observations. The source shows pulsations with a period of 693 s both in…

Astrophysics · Physics 2009-11-07 F. Haberl , C. Motch , F. -J. Zickgraf

We report results of a BeppoSAX observation of the low-mass X-ray binary (LMXB) dipping source XB 1916-053. The source joins the small group of LMXB detected at energies ~100 keV. The non-dip spectrum is well fitted by an absorbed blackbody…