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Following an extensive survey of the galactic plane by the INTEGRAL satellite, new hard X-ray sources are discovered with a significant fraction of Cataclysmic Variables (CVs) among them. We report here the identification of one of these…

天体物理学 · 物理学 2009-11-13 J. M. Bonnet-Bidaud , D. de Martino , M. Falanga , M. Mouchet , N. Masetti

We analyse Chandra, XMM-Newton and HST data of the double-nucleus Ultraluminous Infrared Galaxy (ULIRG), Mrk463. The Chandra detection of two luminous ($\mathrm{L}_\mathrm{2-10 keV}=1.5\times10^{43}$ and $3.8\times10^{42}$ erg cm$^{-2}$…

天体物理学 · 物理学 2009-11-13 Stefano Bianchi , Marco Chiaberge , Enrico Piconcelli , Matteo Guainazzi , Giorgio Matt

Results of analysis of RXTE observations of strongly absorbed X-ray sources IGR J16318-4848 and IGR J16358-4726 are presented. Careful subtraction of Galactic ridge emission contribution to the observed spectra of RXTE/PCA allowed us to…

天体物理学 · 物理学 2009-11-07 M. Revnivtsev

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

IGR J16493-4348 was one of the first new sources to be detected by the INTEGRAL gamma-ray telescope in the 18-100 keV energy band. Based upon spatial coincidence the source was originally associated with the free radio pulsar PSR…

天体物理学 · 物理学 2009-11-13 A. B. Hill , A. J. Dean , R. Landi , V. A. McBride , A. De Rosa , A. J. Bird , A. Bazzano , V. Sguera

In this paper we report the discovery and detailed radio/X-ray analysis of a peculiar giant radio galaxy (GRG) detected by INTEGRAL, IGR J14488-4008. The source has been recently classified as a Seyfert 1.2 galaxy at redshift 0.123; the…

The Seyfert 1.9 galaxy MCG-05-23-016 has been shown to exhibit a complex X-ray spectrum. This source has moderate X-ray luminosity, hosts a comparably low-mass black hole, but accretes at a high Eddington rate, and allows us to study a…

AX J1845.0-0433 is a transient high-mass X-ray binary discovered by ASCA. The source displays bright and short flares observed recently with INTEGRAL. The transient behaviour and the bright and short flares are studied in order to…

天体物理学 · 物理学 2009-11-13 J. A. Zurita Heras , R. Walter

We have carried out a deep survey of the M81 field in the 25-60 keV energy band based on long-term (2003-2023) INTEGRAL observations. A record sensitivity of 0.16 mCrab at a detection significance of 4 sigma has been achieved in the central…

高能天体物理现象 · 物理学 2024-04-26 R. Krivonos , I. Mereminskiy , S. Sazonov

We report Chandra observations of a double X-ray source in the z=0.1569 galaxy SDSS J171544.05+600835.7. The galaxy was initially identified as a dual AGN candidate based on the double-peaked [O III] emission lines, with a line-of-sight…

宇宙学与河外天体物理 · 物理学 2012-06-19 Julia M. Comerford , David Pooley , Brian F. Gerke , Greg M. Madejski

Models for the origin of the hard X-ray background have suggested that sources with the most accretion activity lie hidden in highly obscured AGN. We report on our study of hard, serendipitous sources in the fields of Chandra clusters with…

天体物理学 · 物理学 2007-05-23 P. Gandhi , A. C. Fabian , C. S. Crawford

We report here on near infrared observations of the field around IGR J16358-4756. The source belongs to the new class of highly absorbed X-ray binaries discovered by IBIS/INTEGRAL. Our primary goal was to identify the infrared counterpart…

A new type of high-energy binary systems has been revealed by the INTEGRAL satellite. These sources are in the course of being unveiled by means of multi-wavelength optical, near- and mid-infrared observations. Among these sources, two…

天体物理学 · 物理学 2007-10-02 Sylvain Chaty

We investigate signs of Active Galactic Nucleus (AGN) in the luminous infrared galaxy NGC 3256 at both infrared and X-ray wavelengths. NGC 3256 has double, the Northern and Southern, nuclei (hereafter, N and S nuclei, respectively). We show…

星系天体物理 · 物理学 2015-06-03 Youichi Ohyama , Yuichi Terashima , Kazushi Sakamoto

Kiloparsec-scale binary active galactic nuclei (AGNs) signal active supermassive black hole (SMBH) pairs in merging galaxies. Despite their significance, unambiguously confirmed cases remain scarce and most have been discovered…

宇宙学与河外天体物理 · 物理学 2015-06-11 Xin Liu , Francesca Civano , Yue Shen , Paul J. Green , Jenny E. Greene , Michael A. Strauss

We present X-ray observations of the ultraluminous infrared galaxy, UGC 5101, thought to contain a buried active galactic nucleus (AGN) based on observations in other wavebands. We detected an absorbed hard component at >3 keV, as well as…

天体物理学 · 物理学 2009-11-10 Masatoshi Imanishi , Yuichi Terashima , Naohisa Anabuki , Takao Nakagawa

The International Gamma-Ray Astrophysics Laboratory (INTEGRAL) continues to successfully work in orbit after its launch in 2002. The mission provides the deepest ever survey of hard X-ray sources throughout the Galaxy at energies above 20…

高能天体物理现象 · 物理学 2017-07-26 Roman Krivonos , Sergey Tsygankov , Ilya Mereminskiy , Alexander Lutovinov , Sergey Sazonov , Rashid Sunyaev

We present first INTEGRAL and XMM-Newton observations of a Seyfert galaxy, the type 2 AGN NGC 4388. Several INTEGRAL observations performed in 2003 allow us to study the spectrum in the 20 - 300 keV range. In addition two XMM-Newton…

天体物理学 · 物理学 2009-11-10 V. Beckmann , N. Gehrels , P. Favre , R. Walter , T. J. -L. Courvoisier , P. -O. Petrucci , J. Malzac

We report a Chandra observation of the z=3.395 radio galaxy B2 0902+343. The unresolved X-ray source is centred on the active nucleus. The spectrum is well fit by a flat power law of photon index of Gamma~1.1 with intrinsic absorption of…

天体物理学 · 物理学 2009-11-07 A. C. Fabian , C. S. Crawford , K. Iwasawa

We present results from a Chandra X-ray Observatory study of the field X-ray source population in the vicinity of the radio galaxy MRC 1138-262. Many serendipitous X-ray sources are detected in an area of 8'x8' around the radio source and…

天体物理学 · 物理学 2009-11-07 L. Pentericci , J. D. Kurk , C. L. Carilli , D. E. Harris , G. K. Miley , H. J. A. Rottgering