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相关论文: Revisiting the relativistic ejection event in XTE …

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We report on RXTE observations of the microquasar XTE J1550-564 during a ~70 day outburst in April-June 2000. We study the evolution of the PCA+HEXTE spectra over the outburst. The source transited from an initial Low Hard State (LS), to an…

天体物理学 · 物理学 2016-08-30 J. Rodriguez , S. Corbel , J. A. Tomsick

We present 5-GHz MERLIN radio images of the microquasar GRS 1915+105 during two separate outbursts in 2001 March and 2001 July, following the evolution of the jet components as they move outwards from the core of the system. Proper motions…

Relativistic jets are streams of plasma moving at appreciable fractions of the speed of light. They have been observed from stellar mass black holes ($\sim$3$-$20 solar masses, M$_\odot$) as well as supermassive black holes…

高能天体物理现象 · 物理学 2013-11-28 Natalie Webb , David Cseh , Emil Lenc , Olivier Godet , Didier Barret , Stephane Corbel , Sean Farrell , Rob Fender , Neil Gehrels , Ian Heywood

We present a progress report on MERLIN radio imaging of a radio outburst from GRS 1915+105. The major ejection occurred at the end of an approximately 20-day `plateau' state, characterised by low/hard X-ray fluxes and a relatively strong…

On December 27th 2000 during our regular SMC monitoring program with Rossi X-ray Timing Explorer, strong pulsations were detected with a period of 4.78 seconds. Subsequent slew observations performed on Jan 9th and 13th across the field of…

天体物理学 · 物理学 2009-11-07 S. Laycock , R. H. D. Corbet , M. J. Coe , F. E. Marshall , C. Markwardt , W. Edge , .

The nearby accreting neutron star binary Sco X-1 is the closest example of ongoing relativistic jet production at high Eddington ratios. Previous radio studies have revealed that alongside mildly relativistic, radio-emitting ejecta, there…

高能天体物理现象 · 物理学 2018-12-19 S. E. Motta , R. P. Fender

We have observed an unusually strong X-ray burst as a part of our regular eclipse timing observations of the low mass binary system EXO0748-676. The burst peak flux was 5.2x10^-8 ergs cm^-2 s^-1, approximately five times the normal peak…

天体物理学 · 物理学 2009-11-13 Michael T. Wolff , Peter A. Becker , Paul S. Ray , Kent S. Wood

We have carried out a thorough optical study of the closest star formation jet. The inner arcminute surrounding the class 0/I binary protostar L1551 IRS5 and its associated jet (HH154) have been observed using the Hubble Space Telescope…

天体物理学 · 物理学 2009-11-10 C. V. M. Fridlund , R. Liseau , A. A. Djupvik , M. Huldtgren , Glenn. J. White , F. Favata , G. Giardino

We present an analysis of the high frequency timing properties of the April-May 2000 outburst of the black hole candidate and Galactic microquasar XTE J1550-564, measured with the Rossi X-ray Timing Explorer. The rapid X-ray variability we…

We analysed Rossi X-ray Timing Explorer observations of the accretion-powered 401 Hz pulsar SAX J1808.4-3658, in order to precisely determine the source distance. While the fluences for the five transient outbursts observed from 1996 were…

天体物理学 · 物理学 2011-02-11 Duncan Galloway , Andrew Cumming

Obtaining simultaneous radio and X-ray data during the outburst decay of soft X-ray transients is a potentially important tool to study the disc - jet connection. Here we report results of the analysis of (nearly) simultaneous radio (VLA or…

天体物理学 · 物理学 2009-11-10 P. G. Jonker , E. Gallo , V. Dhawan , M. Rupen , R. P. Fender , G. Dubus

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…

天体物理学 · 物理学 2009-11-07 S. Campana , L. Stella , T. Belloni , G. L. Israel , A. Santangelo , F. Frontera , M. Orlandini , D. Dal Fiume

We present the radio and X-ray monitoring campaign of the 2019/2020 outburst of MAXI J1348-630, a new black hole X-ray binary (XRB) discovered in 2019 January. We observed MAXI J1348-630 for $\sim$14 months in the radio band with MeerKAT…

We present multi-frequency monitoring observations of the black hole X-ray binary V404 Cygni throughout its June 2015 outburst. Our data set includes radio and mm/sub-mm photometry, taken with the Karl G. Jansky Very Large Array, Arc-Minute…

We present radio imaging observations of the 1998 outburst of the peculiar emission line star CI Cam, taken about 1, 4, 75, 82, 93, 163, and 306 days after the beginning of the 31.64 March 1998 X-ray flare. The first two epochs show a…

天体物理学 · 物理学 2009-11-10 Amy J. Mioduszewski , Michael P. Rupen

XTE J1908+094 is an X-ray transient that went into outburst in February 2002. After two months it reached a 2-250 keV peak flux of 1 to 2 X 10-8 erg/s/cm2. Circumstantial evidence points to an accreting galactic black hole as the origin of…

天体物理学 · 物理学 2009-11-07 J. J. M. in 't Zand , J. M. Miller , T. Oosterbroek , A. N. Parmar

Tidal disruption events (TDEs) are transient, multi-wavelength events in which a star is ripped apart by a supermassive black hole. Observations show that in a small fraction of TDEs, a short-lived, synchrotron emitting jet is produced. We…

We report multifrequency radio observations of GRO J1655-40 obtained with the Australia Telescope Compact Array, the Molonglo Observatory Synthesis Telescope and the Hartebeesthoek Radio Astronomy Observatory at the time of the major hard…

天体物理学 · 物理学 2009-10-31 D. C. Hannikainen , R. W. Hunstead , D. Campbell-Wilson , K. Wu , D. J. McKay , D. P. Smits

MAXI J1836-194 is a Galactic black hole candidate X-ray binary that was discovered in 2011 when it went into outburst. In this paper, we present the full radio monitoring of this system during its `failed' outburst, in which the source did…

We report the discovery of transient radio emission from the nearby optically-discovered TDE ASASSN-14li (distance of 90 Mpc), making it the first typical TDE detected in the radio, and unambiguously pointing to the formation of a…

高能天体物理现象 · 物理学 2016-03-16 Kate D. Alexander , Edo Berger , James Guillochon , Bevin A. Zauderer , Peter K. G. Williams