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Two \textit{NuSTAR} observations of the luminous X-ray pulsar LMC X-4 in October and November 2015 captured several bright accretion flares from this source, which has a long history of stable pulse and superorbital behavior. We present a…

CXOU J110926.4-650224 is a candidate transitional millisecond pulsar (tMSP) with X-ray and radio emission properties reminiscent of those observed in confirmed tMSPs in their X-ray 'subluminous' disc state. We present the results of…

We present the results of two extensive Rossi X-ray Timing Explorer observations of large X-ray flaring episodes from the high-mass X-ray binary pulsar LMC X-4. Light curves during the flaring episodes comprise bright peaks embedded in…

天体物理学 · 物理学 2009-11-07 Dae-Sik Moon , Stephen S. Eikenberry , Ira M. Wasserman

We report the discovery of two new Galactic accreting compact objects consistent with the respective positions of the unassociated Fermi-LAT gamma-ray sources 4FGL J0639.1--8009 and 4FGL J1824.2+1231. A combination of new and archival X-ray…

高能天体物理现象 · 物理学 2025-04-17 Rebecca Kyer , Subhroja Roy , Jay Strader , Ryan Urquhart , Isabella Molina , Peter Craig , Laura Chomiuk

In this paper, we report on the analysis of the peculiar X-ray variability displayed by the accreting millisecond X-ray pulsar IGR J00291+5934 in a 80 ks-long joint NuSTAR and XMM-Newton observation performed during the source outburst in…

高能天体物理现象 · 物理学 2017-01-18 C. Ferrigno , E. Bozzo , A. Sanna , F. Pintore , A. Papitto , A. Riggio , L. Burderi , T. Di Salvo , R. Iaria , A. D'Aì

Transitional millisecond pulsars are systems that alternate between an accreting low-mass X-ray binary (LMXB) state, and a non-accreting radio pulsar state. When at the LMXB state, their X-ray and optical light curves show rapid flares and…

高能天体物理现象 · 物理学 2017-12-27 Pasi Hakala , Jari J. E. Kajava

The Fermi $\gamma$-ray source 1FGL J1417.7--4407 (J1417) is a compact X-ray binary with a neutron star primary and a red giant companion in a $\sim$5.4 day orbit. This initial conclusion, based on optical and X-ray data, was confirmed when…

We present the first detection of X-ray coherent pulsations from the transitional millisecond pulsar XSS J12270-4859, while it was in a sub-luminous accretion disk state characterized by a 0.5-10 keV luminosity of 5E33 erg/s (assuming a…

高能天体物理现象 · 物理学 2015-07-24 A. Papitto , D. de Martino , T. M. Belloni , M. Burgay , A. Pellizzoni , A. Possenti , D. F. Torres

We present coordinated Chandra X-ray Observatory and Karl G. Jansky Very Large Array observations of the transitional millisecond pulsar PSR J1023+0038 in its low-luminosity accreting state. The unprecedented five hours of strictly…

The spectra of several X-ray binary pulsars display a clear soft excess, which in most cases can be described with a blackbody model, above the main power-law component. While in the high-luminosity sources it is usually characterized by…

高能天体物理现象 · 物理学 2015-05-13 N. La Palombara , L. Sidoli , P. Esposito , A. Tiengo , S. Mereghetti

We present Karl G. Jansky Very Large Array radio frequency observations of the new accreting millisecond X-ray pulsar (AMXP), IGR J16597$-$3704, located in the globular cluster NGC 6256. With these data, we detect a radio counterpart to IGR…

IGR~J18245--2452/PSR J1824--2452I is one of the rare transitional accreting millisecond X-ray pulsars, showing direct evidence of switches between states of rotation powered radio pulsations and accretion powered X-ray pulsations, dubbed…

高能天体物理现象 · 物理学 2017-07-19 V. De Falco , L. Kuiper , E. Bozzo , C. Ferrigno , J. Poutanen , L. Stella , M. Falanga

IGR J17407-2808 is an enigmatic and poorly studied X-ray binary that was recently observed quasi-simultaneously with NuSTAR and XMM-Newton. In this paper we report the results of this observational campaign. During the first 60 ks of…

高能天体物理现象 · 物理学 2023-06-14 L. Ducci , C. Malacaria , P. Romano , E. Bozzo , M. Berton , A. Santangelo , E. Congiu

We present an extensive radio monitoring campaign of the nuclear transient eRASSt J234403-352640 with the Australia Telescope Compact Array, one of the most X-ray luminous TDE candidates discovered by the SRG/eROSITA all-sky survey. The…

高能天体物理现象 · 物理学 2024-01-31 A. J. Goodwin , G. E. Anderson , J. C. A. Miller-Jones , A. Malyali , I. Grotova , D. Homan , A. Kawka , M. Krumpe , Z. Liu , A. Rau

We report the detection of 376.05 Hz (2.66 ms) coherent X-ray pulsations in NICER observations of a transient outburst of the low-mass X-ray binary IGR J17494-3030 in 2020 October/November. The system is an accreting millisecond X-ray…

In this work, we studied X-ray source SRGe~J021932.4$-$040154 (SRGe J021932), which we associated with a single X-ray active star of spectral class G2V-G4V and the rotational period $\rm P_{rot} < 9.3$ days. Additional analysis of TESS…

Understanding the formation and properties of relativistic jets from accreting compact objects has far-reaching implications in astrophysics. Transitional millisecond pulsars (tMSPs) - a class of neutron stars transitioning between radio…

高能天体物理现象 · 物理学 2025-03-28 K. I. I. Koljonen , M. Linares , J. C. A. Miller-Jones

We present an optical (gri) study during quiescence of the accreting millisecond X-ray pulsar IGR J00291+5934 performed with the 10.4m Gran Telescopio Canarias (GTC) in August 2014. Despite the source being in quiescence at the time of our…

高能天体物理现象 · 物理学 2017-04-12 M. C. Baglio , S. Campana , P. D'Avanzo , A. Papitto , L. Burderi , T. Di Salvo , T. Muñoz Darias , N. Rea , D. F. Torres

We report on the extreme behaviour of the high redshift blazar GB B1428+4217 at z=4.72. A continued programme of radio measurements has revealed an exceptional flare in the lightcurve, with the 15.2 GHz flux density rising by a factor ~3…

天体物理学 · 物理学 2009-09-17 M. A. Worsley , A. C. Fabian , G. G. Pooley , C. J. Chandler

We have discovered a new candidate redback millisecond pulsar binary near the center of the error ellipse of the bright unassociated Fermi-LAT $\gamma$-ray source 4FGL J0940.3-7610. The candidate counterpart is a variable optical source…

高能天体物理现象 · 物理学 2021-03-24 Samuel J. Swihart , Jay Strader , Elias Aydi , Laura Chomiuk , Kristen C. Dage , Laura Shishkovsky