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We analyzed the zero-order image of a 50 ks Chandra gratings observation of Circinus X-1, taken in 2005 during the source's low-flux state. Circinus X-1 is an accreting neutron star that exhibits ultra-relativistic arcsecond-scale radio…

天体物理学 · 物理学 2009-11-13 S. Heinz , N. S. Schulz , W. N. Brandt , D. K. Galloway

In observations with the Australia Telescope Compact Array we have resolved the radio counterpart of the unusual X-ray binary Cir X-1 into an asymmetric extended structure on arcsecond scales. In order to quantify the asymmetry we have…

We present observations of the neutron star X-ray binary and relativistic jet source Circinus X-1 made at 4.8 and 8.6 GHz with the Australia Telescope Compact Array during a time interval of almost 10 years. The system shows significant…

天体物理学 · 物理学 2009-11-13 V. Tudose , R. P. Fender , A. K. Tzioumis , R. E. Spencer , M. van der Klis

Accretion conditions and morphologies of X-ray transients containing neutron stars are still poorly understood. Circinus X-1 is an enigmatic case where we observe X-ray flux changes covering four orders of magnitude. We observed Circinus…

高能天体物理现象 · 物理学 2020-03-25 N. S. Schulz , T. E. Kallman , S. Heinz , P. Sell , P. Jonker , W. N. Brandt

We report the discovery of multi-scale X-ray jets from the accreting neutron star X-ray binary, Circinus X-1. The bipolar outflows show wide opening angles and are spatially coincident with the radio jets seen in new high-resolution radio…

We present results from the first successful millimetre (combined 33 GHz and 35 GHz) observations of the neutron star X-ray binary Circinus X-1, using the Australia Telescope Compact Array. The source was clearly detected in all three…

高能天体物理现象 · 物理学 2015-05-30 D. E. Calvelo , R. P. Fender , A. K. Tzioumis , J. W. Broderick

We present the results of simultaneous X-ray and radio observations of the peculiar Z-type neutron star X-ray binary Cir X-1, observed with the Rossi X-ray timing explorer satellite and the Australia Telescope Compact Array in 2000 October…

高能天体物理现象 · 物理学 2015-05-13 Paolo Soleri , Valeriu Tudose , Rob Fender , Michiel van der Klis , Peter G. Jonker

We present results from the first radio observations of a complete orbit (~ 17 days) of the neutron star X-ray binary Circinus X-1 using the Australia Telescope Compact Array Broadband Backend, taken while the system was in an historically…

高能天体物理现象 · 物理学 2015-05-30 D. E. Calvelo , R. P. Fender , A. K. Tzioumis , N. Kawai , J. W. Broderick , M. E. Bell

We present the results of millimetre (33 and 35 GHz) and centimetre (2.1, 5.5 and 9.0 GHz) wavelength observations of the neutron star X-ray binary Circinus X-1, using the Australia Telescope Compact Array. We have used advanced calibration…

高能天体物理现象 · 物理学 2019-01-16 M. Coriat , R. Fender , C. Tasse , O. Smirnov , A. K. Tzioumis , J. W. Broderick

We have used the Chandra X-ray Observatory to resolve spatially and spectrally the X-ray emission from the Circinus Galaxy. We report here on the nature of the X-ray emission from the off-nuclear point sources associated with the disk of…

天体物理学 · 物理学 2009-11-06 F. E. Bauer , W. N. Brandt , R. M. Sambruna , G. Chartas , G. P. Garmire , S. Kaspi , H. Netzer

Circinus X-1 is a neutron-star-accreting X-ray binary in a wide (P$_{\rm orb}$ = 16.6 d), eccentric orbit. After two years of relatively low X-ray luminosity, in May 2010 Circinus X-1 went into outburst, reaching 0.4 Crab flux. This…

高能天体物理现象 · 物理学 2015-06-04 A. D'Aì , E. Bozzo , A. Papitto , R. Iaria , T. Di Salvo , L. Burderi , A. Riggio , E. Egron , N. R. Robba

We report on a recent Chandra ACIS-S observation of the Circinus galaxy. These observations confirm that the nuclear spectrum results from reflection of a hard X-ray continuum by ``neutral'' matter. The nuclear X-ray emission is extended by…

天体物理学 · 物理学 2009-11-06 David A. Smith , Andrew S. Wilson

Precessing relativistic jets launched by compact objects are rarely directly measured, and present an invaluable opportunity to better understand many features of astrophysical jets. In this Letter we present MeerKAT radio observations of…

Chandra High Energy Transmission Grating Spectrometer (HETGS) observations of the extremely luminous and violent X-ray binary Cir X-1 reveal many X-ray emission lines showing broad P Cygni profiles. These are from H-like and He-like ions of…

天体物理学 · 物理学 2007-05-23 N. S. Schulz , W. N. Brandt

New radio observations of the radio-jet X-ray binary Circinus X-1 over nearly an entire 16.6-day orbit are presented. The source continues to undergo radio flaring in the phase interval 0.0 - 0.2 and appears to be brightening since…

天体物理学 · 物理学 2009-10-30 R. P. Fender

We present the first grating-resolution X-ray spectra of the X-ray binary Cir X-1, obtained with the High Energy Transmission Grating Spectrometer on Chandra. These reveal a rich set of lines from H-like and/or He-like Ne, Mg, Si, S and Fe…

天体物理学 · 物理学 2009-10-31 W. N. Brandt , N. S. Schulz

Circinus X-1 (Cir X-1) is a neutron star binary with an elliptical orbit of 16.6~days. The source is unique for its extreme youth, providing a key to understanding early binary evolution. However, its X-ray variability is too complex to…

高能天体物理现象 · 物理学 2023-11-15 Mayu Tominaga , Masahiro Tsujimoto , Ken Ebisawa , Teruaki Enoto , Kimitake Hayasaki

We present the first resolved imaging of the milliarcsecond-scale jets in the neutron star X-ray binary Circinus X-1, made using the Australian Long Baseline Array. The angular extent of the resolved jets is ~20 milliarcseconds,…

We present a partial analysis of a multi-wavelength study of the X-ray binary Cir X-1, a system harboring the most relativistic outflow in our galaxy so far. The data were taken (almost) simultaneously in radio and X ray during a survey…

天体物理学 · 物理学 2009-04-14 V. Tudose , P. Soleri , R. P. Fender , P. G. Jonker , M. van der Klis , A. K. Tzioumis , R. E. Spencer

We present multi-epoch observations of the radio nebula around the neutron star X-ray binary Circinus X-1 made at 1.4 and 2.5 GHz with the Australia Telescope Compact Array between October 2000 and September 2004. The nebula can be seen as…

天体物理学 · 物理学 2009-11-11 V. Tudose , R. P. Fender , C. R. Kaiser , A. K. Tzioumis , M. van der Klis , R. Spencer
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