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相关论文: Broadband X-ray spectrum of intermediate polar V12…

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We present results of an analysis of broadband spectra of 14 intermediate polars obtained with the RXTE observatory (PCA and HEXTE spectrometers, 3-100 keV). By means of our calculations of the structure and the emergent spectrum of the…

天体物理学 · 物理学 2009-11-10 V. Suleimanov , M. Revnivtsev , H. Ritter

We present the hard X-ray time-averaged spectrum of the intermediate polar V709 Cas observed with INTEGRAL. We performed the observation using data from the IBIS/ISGRI instrument in the 20-100 keV energy band and from JEM-X at lower energy…

天体物理学 · 物理学 2009-11-11 M. Falanga , J. M. Bonnet-Bidaud , V. Suleimanov

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

The analysis of the third INTEGRAL/IBIS survey has revealed several new cataclysmic variables, most of which turned out to be intermediate polars, thus confirming that these objects are strong emitters in hard X-rays. Here we present high…

天体物理学 · 物理学 2009-11-13 R. Landi , L. Bassani , A. J. Dean , A. J. Bird , M. Fiocchi , A. Bazzano , J. A. Nousek , J. P. Osborne

Aims. To determine the credentials of nine candidate intermediate polars in order to confirm whether or not they are magnetic cataclysmic variables. Methods. Frequency analysis of RXTE and XMM data was used to search for temporal variations…

太阳与恒星天体物理 · 物理学 2015-05-20 O. W. Butters , A. J. Norton , K. Mukai , J. A. Tomsick

We present the results of our optical identification of the X-ray source IGR J16547-1916 detected by the INTEGRAL observatory during a deep all-sky survey. Analysis of the spectroscopic data from the SWIFT and INTEGRAL observatories in the…

高能天体物理现象 · 物理学 2015-05-20 A. Lutovinov , R. Burenin , M. Revnivtsev , V. Suleimanov , A. Tkachenko

We derive the spectra of the cosmic X-ray background (CXB) and of the Galactic ridge X-ray emission (GRXE) in the ~20-200 keV range from the data of the IBIS instrument aboard the INTEGRAL satellite obtained during the four dedicated…

宇宙学与河外天体物理 · 物理学 2015-05-14 M. Turler , M. Chernyakova , T. J. -L. Courvoisier , P. Lubinski , A. Neronov , N. Produit , R. Walter

White dwarf masses in cataclysmic variables are difficult to determine accurately, but are fundamental for understanding binary system parameters, as well as binary evolution. We investigate the X-ray spectral properties of a sample of…

星系天体物理 · 物理学 2009-11-13 Jorg Brunschweiger , Jochen Greiner , Marco Ajello , Julian Osborne

We present X-ray observations of the periodic optical source ZTF J185139.81+171430.3 (hereafter ZTF J1851) by the XMM, NICER and NuSTAR telescopes. The source was initially speculated to be a white dwarf (WD) pulsar system due to its short…

高能天体物理现象 · 物理学 2025-11-25 Ren Deng , Kaya Mori , Eric Miao , Gabriel Bridges , Charles J. Hailey , David A. H. Buckley , Gavin Ramsay , Dan Jarvis

We present broad-band (0.1--90keV) spectral and temporal properties of the three Intermediate Polars, RE0751+144 (PQ Gem), RXJ0558.0+5353 (V405Aur) and RXJ1712.6-2414 (V2400 Oph) based on simultaneous soft and hard X-ray observations with…

天体物理学 · 物理学 2009-11-10 D. de Martino , G. Matt , T. Belloni , F. Haberl , K. Mukai

The majority of cataclysmic variables observed in the hard X-ray energy band are intermediate polars where the magnetic field is strong enough to channel the accreting matter to the magnetic poles of the white dwarf. A shock above the…

天体物理学 · 物理学 2008-11-27 V. Suleimanov , J. Poutanen , M. Falanga , K. Werner

Using X-ray observations from the NuSTAR and Swift satellites, we present temporal and spectral properties of an intermediate polar (IP) IGR J16547-1916. A persistent X-ray period at ~ 546 s confirming the optical spin period obtained from…

高能天体物理现象 · 物理学 2022-01-05 A. Joshi , W. Wang , J. C. Pandey , K. P. Singh , S. Naik , A. Raj , G. C. Anupama , N. Rawat

We report the discovery of persistent hard X-ray emission extending up to 150 keV from the soft gamma-ray repeater SGR 1806-20 using data obtained with the INTEGRAL satellite in 2003-2004. Previous observations of hard X-rays from objects…

天体物理学 · 物理学 2009-11-10 S. Mereghetti , D. Gotz , I. F. Mirabel , K. Hurley

We present RXTE and BeppoSAX observations of the Intermediate Polar V709 Cas acquired in 1997 and 1998 respectively. The X-ray emission from 0.1 to 30keV is dominated by the strong pulsation at the rotational period of the white dwarf…

We report the first detailed spectroscopic observations of the recently identified intermediate polar RXJ0028.8+5917/V709 Cas. We discovered that the system shows significant EW ~ (2-4)A broad absorptions, affecting the Balmer lines from…

天体物理学 · 物理学 2007-05-23 J. M. Bonnet-Bidaud , M. Mouchet , D. de Martino , G. Matt , C. Motch

A significant number of cataclysmic variables were detected as hard X-ray sources in the INTEGRAL survey, most of them of the magnetic intermediate polar type. We present a detailed X-ray broad-band study of two new sources, IGR J00234+6141…

太阳与恒星天体物理 · 物理学 2010-07-21 G. Anzolin , D. de Martino , M. Falanga , K. Mukai , J. -M. Bonnet-Bidaud , M. Mouchet , Y. Terada , M. Ishida

ASCA and GINGA X-ray data from the magnetic Cataclysmic Variable BY Cam show that the spectrum is strongly affected by complex absorption, probably from the pre-shock accretion column. The intrinsic emission from the shock is significantly…

天体物理学 · 物理学 2015-06-24 C. Done , P. Magdziarz

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…

天体物理学 · 物理学 2009-11-07 F. Haberl , C. Motch , F. -J. Zickgraf

We present results of spectral and timing analysis of the fast X-ray transient XTE J1901+014 based on data of the RXTE and INTEGRAL observatories. With the INTEGRAL/ISGRI the source was detected at a significance level of 20$\sigma$ with…

天体物理学 · 物理学 2007-05-23 D. I. Karasev , A. A. Lutovinov , S. A. Grebenev

A simultaneous broadband analysis of X-ray data obtained with XMM-Newton and NuSTAR observatories for the asynchronous polar source CD Ind is presented. The spin folded lightcurve in soft 0.3-3.0 keV band shows single broad hump-like…

高能天体物理现象 · 物理学 2022-03-07 Anirban Dutta , Vikram Rana
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