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Black widows and redbacks are binary systems consisting of a millisecond pulsar in a close binary with a companion having matter driven off of its surface by the pulsar wind. X-rays due to an intra-binary shock have been observed from many…

We present observations of fields containing eight recently discovered binary millisecond pulsars using the telescopes at MDM Observatory. Optical counterparts to four of these systems are detected, one of which, PSR J2214+3000, is a novel…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Joshua Schroeder , Jules Halpern

In the latest data release from the Fermi $\gamma$-ray Space Telescope (the 4th Fermi LAT 14 yr Catalog, or 4FGL), more than 50% of the Galactic sources are yet to be identified. We observed 13 unidentified Fermi LAT sources with the…

High Energy Astrophysical Phenomena · Physics 2024-08-30 Blagoy Rangelov , Hui Yang , Brice Williams , Oleg Kargaltsev , Jeremy Hare , Kean Martinic

During a search for coherent signals in the X-ray archival data of XMM-Newton, we discovered a modulation at 1.2 s in 3XMM J004301.4+413017 (3X J0043), a source lying in the direction of an external arm of M 31. This short period indicates…

We have studied the variability of the black-widow type binary millisecond pulsar PSR J1311$-$3430 from optical to gamma-ray energies. We confirm evidence for orbital modulation in the weak off-pulse $\ge$200-MeV emission, with a peak at…

High Energy Astrophysical Phenomena · Physics 2017-12-06 Hongjun An , Roger W. Romani , Tyrel Johnson , Matthew Kerr , Colin J. Clark

We report the discovery of a dark companion to 2MASS J15274848+3536572 with an orbital period of 6.14 hr. Combining the radial velocity from LAMOST observations and modelling of the multiband light curve, one obtains a mass function of…

The EXTraS project to explore the X-ray Transient and variable Sky searches for coherent signals in the X-ray archival data of XMM-Newton. XMM-Newton performed more than 400 pointed observations in the region of the Large Magellanic Cloud…

We report results of the first detailed spectral and temporal studies of the recently discovered Be/X-ray binary eRASSU J050810.4$-$660653 in LMC based on the data from the SRG/ART-XC, NuSTAR and Swift/XRT instruments obtained in December…

We present X-ray, ultraviolet, and optical observations of 1RXS J154439.4-112820, the most probable counterpart of the unassociated Fermi LAT source 3FGL J1544.6-1125. The optical data reveal rapid variability, which is a feature of…

High Energy Astrophysical Phenomena · Physics 2015-06-24 Slavko Bogdanov , Jules P. Halpern

The 559 Hz black-widow pulsar PSR J1555-2908, originally discovered in radio, is also a bright gamma-ray pulsar. Timing its pulsations using 12 yr of Fermi-LAT gamma-ray data reveals long-term variations in its spin frequency that are much…

High Energy Astrophysical Phenomena · Physics 2022-06-01 L. Nieder , M. Kerr , C. J. Clark , P. Bruel , H. T. Cromartie , S. M. Ransom , P. S. Ray

Black widows are millisecond pulsars with low-mass companions, a few per cent the mass of the sun, on orbits of several hours. These companions are presumably the remnants of main sequence stars that lost their mass through a combination of…

High Energy Astrophysical Phenomena · Physics 2020-12-07 Sivan Ginzburg , Eliot Quataert

The Burst Alert Telescope (BAT) on board Swift has accumulated extensive light curves for 265 sources (not including GRBs) in the energy range 14 to 200 keV. We present here a summary of searches for periodic modulation in the flux from…

This paper presents analysis and interpretation of OGLE photometric data of four X-ray binary pulsar systems in the Small Magellanic Cloud: 1WGA J0054.9-7226, RX J0050.7-7316, RX J0049.1-7250, and 1SAX J0103.2-7209. In each case, the…

Astrophysics · Physics 2009-10-31 M. J. Coe , J. A. Orosz

We have presented the first joint {\it XMM-Newton} and {\it NuSTAR} analysis of the millisecond pulsar (MSP) binary PSR J1653$-$0158. The 75-minute orbital period inferred from optical and gamma-ray observations together with the 1.97-ms…

High Energy Astrophysical Phenomena · Physics 2022-06-14 Jane SiNan Long , Albert K. H. kong , Kinwah Wu , Jumpei Takata , Qin Han , David C. Y. Hui , Kwan Lok Li

We report on the detection of X-ray pulsations at 2.1 ms from the known X-ray burster IGR J17379-3747 using XMM-Newton. The coherent signal shows a clear Doppler modulation from which we estimate an orbital period of ~1.9 hours and a…

High Energy Astrophysical Phenomena · Physics 2018-09-05 A. Sanna , E. Bozzo , A. Papitto , A. Riggio , C. Ferrigno , T. Di Salvo , R. Iaria , S. M. Mazzola , N. D'Amico , L. Burderi

I present a 40 kilosecond Nuclear Spectroscopic Telescope Array (NuSTAR) observation of the recently identified low-luminosity X-ray binary and transitional millisecond pulsar (tMSP) candidate 1RXS J154439.4-112820, which is associated with…

High Energy Astrophysical Phenomena · Physics 2016-07-27 Slavko Bogdanov

We present the results of precision gamma-ray timing measurements of the binary millisecond pulsar PSR J2339$-$0533, an irradiating system of "redback" type, using data from the Fermi Large Area Telescope. We describe an optimized analysis…

High Energy Astrophysical Phenomena · Physics 2015-06-30 Holger J. Pletsch , Colin J. Clark

Redback pulsars are a subclass of millisecond pulsar system with a low-mass non-degenerate companion star being ablated by the pulsar. They are of interest due to the insights they can provide for late-stage pulsar evolution during the…

High Energy Astrophysical Phenomena · Physics 2025-11-19 O. A. Johnson , E. F. Keane , D. J. McKenna , H. Qiu , S. J. Swihart , J. Strader , M. McLaughlin

The recent report of a binary companion to the progenitor of supernova 1993J may provide important clues for identifying the nature of the nascent compact object. Given the estimates of the progenitor mass, the potential power source is…

Astrophysics · Physics 2009-11-10 Enrico Ramirez-Ruiz , Aldo M. Serenelli

Gamma-ray binaries are stellar systems containing a neutron star or black hole with gamma-ray emission produced by an interaction between the components. These systems are rare, even though binary evolution models predict dozens in our…

High Energy Astrophysical Phenomena · Physics 2012-02-16 The Fermi LAT Collaboration , M. J. Coe , F. Di Mille , P. G. Edwards , M. D. Filipović , J. L. Payne , J. Stevens , M. A. P. Torres