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Related papers: The extraordinary X-ray spectrum of XTE J0421+560

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We report on a BeppoSAX observation of the transient X-ray source XTE J0421+560 during quiescence performed ~150 days after the 1998 April outburst. The source had an unabsorbed 0.5-10 keV flux of 6.7x10^{-12} erg/cm2/s and was still…

We report on BeppoSAX observations of the X-ray transient XTE J0421+560 in quiescence 156, 541, and ~690 days after the maximum of the 1998 April outburst. In the first observation the source was soft with a power-law photon index of 4.0…

Astrophysics · Physics 2007-05-23 A. N. Parmar , T. Belloni , M. Orlandini , D. Dal Fiume , A. Orr , N. Masetti

We present the results of observations of XTE J0421+560 X-ray transient with Rossi X-ray Timing Explorer in the beginning of April 1998. Lightcurve, obtained by ASM all-sky monitor, shows unusually fast decrease in the object's luminosity.…

Astrophysics · Physics 2007-05-23 M. Revnivtsev , A. Emelyanov , K. Borozdin

We present the results of the analysis of RXTE, BATSE and optical/infrared data of the 1998 outburst of the X-ray transient system XTE J0421+560 (CI Cam). The X-ray outburst shows a very fast decay (initial e-folding time ~0.5 days, slowing…

We report on two X-ray observations of the transient source XTE J0421+560 performed by BeppoSAX, and on a series of observations performed by the 0.7m Teramo-Normale Telescope. Outburst peak occurrence time and duration depend on photon…

We have observed the X-ray transient XTE J0421+56 in quiescence with XMM-Newton. The observed spectrum is highly unusual being dominated by an emission feature at ~6.5 keV. The spectrum can be fit using a partially covered power-law and…

Astrophysics · Physics 2009-11-07 L. Boirin , A. N. Parmar , T. Oosterbroek , D. Lumb , M. Orlandini , N. Schartel

We have observed the soft X-ray transient XTE J0421+56 in quiescence with XMM-Newton. The observed spectrum is highly unusual being dominated by a broad feature at 6.5 keV and can be modeled by a strongly absorbed continuum. The spectra of…

Astrophysics · Physics 2007-05-23 L. Boirin , A. N. Parmar , D. Lumb , M. Orlandini , N. Schartel

We present a detailed X-ray study of the 2003 XMM-Newton observation of the High Mass X-ray Binary XTE J0421+560/CI Cam. The continuum of the X-ray spectrum is well described by a flat power law (Gamma=1.0+/-0.2) with a large intrinsic…

High Energy Astrophysical Phenomena · Physics 2015-06-12 E. S. Bartlett , J. S. Clark , M. J. Coe , M. R. Garcia , P. Uttley

We report on optical spectroscopic observations of the X-ray Transient XTE J1118+480 covering the period from April 7, 2000 to July 4, 2000. The spectrum is characterized by weak, broad, double-peaked Balmer and He lines on top of a blue…

Astrophysics · Physics 2009-10-31 Guillaume Dubus , Rita S. J. Kim , Kristen Menou , Paula Szkody , David V. Bowen

SAX J1747.0-2853 is an X-ray transient which exhibited X-ray outbursts yearly between 1998 and 2001, and most probably also in 1976. The outburst of 2000 was the longest and brightest. We have analyzed X-ray data sets that focus on the 2000…

We have discovered with the Wide Field Cameras on board BeppoSAX the weak transient X-ray source SAXJ2239.3+6116 whose position coincides with that of 4U2238+60/3A2237+608 and is close to that of the fast transient AT2238+60 and the…

SAX J1819.3-2525 is a nearby X-ray transient which exhibited a fast and large X-ray outburst on Sep. 15, 1999 (Smith et al. 1999). The Wide Field Cameras and the Narrow Field Instruments (NFI) on board BeppoSAX observed SAX J1819.3-2525 at…

We report on multi-band observations of the transient source Swift J0840.7-3516, which was detected in outburst in 2020 February by the Neil Gehrels Swift Observatory. The outburst episode lasted just ~5 days, during which the X-ray…

High Energy Astrophysical Phenomena · Physics 2021-06-09 F. Coti Zelati , A. de Ugarte Postigo , T. D. Russell , A. Borghese , N. Rea , P. Esposito , G. L. Israel , S. Campana

We observed the newly discovered Galactic jet source XTE J0421+560 (= CI Cam) with ASCA from 1998 April 3.3 to April 4.1 (UT), three days after the beginning of the outburst. The X-ray intensity in the 1-10 keV band gradually decreased with…

Astrophysics · Physics 2009-10-31 Y. Ueda , M. Ishida , H. Inoue , T. Dotani , J. Greiner , W. H. G. Lewin

We report on the results of a series of X-ray observations of the transient black hole candidate XTE J2012+381 during the 1998 outburst performed with the BeppoSAX satellite. The observed broad-band energy spectrum can be described with the…

On 28 February 2007 a new outburst of the previously known transient source XTE J1856+053 was detected with RXTE/ASM. We present here the results of an XMM-Newton (0.5-10.0 keV) Target of Opportunity observation performed on 14 March 2007,…

Astrophysics · Physics 2011-08-31 G. Sala , J. Greiner , M. Ajello , N. Primak

We present optical photometry and spectroscopy of the X-ray transient XTE J1859+226, obtained during outburst and its subsequent decay to quiescence. Both the X-ray and optical properties are very similar to those of well-studied black hole…

We report on optical and RXTE observations of a new high-latitude bursting X-ray transient, XTE J2123-058. We identified the optical counterpart, measured the 5.9573 hr orbital period and constrained the binary inclination and the source…

Astrophysics · Physics 2009-10-31 John A. Tomsick , Jules P. Halpern , Jonathan Kemp , Philip Kaaret

During observation campaigns of the Galactic Bulge region, BeppoSAX detected a total of 21 new X-ray bursters in about 6 years of operation. These sources are mostly transient and often feature a hard X-ray spectrum, extending up to ~ 200…

Astrophysics · Physics 2007-05-23 L. Natalucci , A. Bazzano , F. Capitanio , M. Cocchi , P. Ubertini , J. J. M. in 't Zand

We present time-resolved spectroscopy of the soft X-ray transient XTE J2123-058 in outburst. A useful spectral coverage of 3700-6700A was achieved spanning two orbits of the binary, with single epoch coverage extending to \~9000A. The…

Astrophysics · Physics 2015-06-24 R. I. Hynes , P. A. Charles , C. A. Haswell , J. Casares , C. Zurita , M. Serra-Ricart
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