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Transitional millisecond pulsars (tMSPs) represent a dynamic category of celestial sources that establish a crucial connection between low-mass X-ray binaries and millisecond radio pulsars. These systems exhibit transitions from…

High Energy Astrophysical Phenomena · Physics 2024-09-20 M. M. Messa , P. D'Avanzo , F. Coti Zelati , M. C. Baglio , S. Campana

We present the discovery of a new optical/X-ray source likely associated with the Fermi $\gamma$-ray source 4FGL J1408.6-2917. Its high-amplitude periodic optical variability, large spectroscopic radial velocity semi-amplitude, evidence for…

High Energy Astrophysical Phenomena · Physics 2023-01-04 Samuel J. Swihart , Jay Strader , Laura Chomiuk , Elias Aydi , Kirill V. Sokolovsky , Paul S. Ray , Matthew Kerr

We report the identification from multi-wavelength observations of the Fermi Large Area Telescope (LAT) source 4FGL J1405.1-6119 (= 3FGL J1405.4-6119) as a high-mass gamma-ray binary. Observations with the LAT show that gamma-ray emission…

High Energy Astrophysical Phenomena · Physics 2019-11-06 R. H. D. Corbet , L. Chomiuk , M. J. Coe , J. B. Coley , G. Dubus , P. G. Edwards , P. Martin , V. A. McBride , J. Stevens , J. Strader , L. J. Townsend

We report the results from our analysis of the \textit{Fermi} Large Area Telescope data of the \textit{Fermi} unassociated source 2FGL J1906.5$+$0720, which is a high-ranked candidate pulsar. In order to better study our target, we first…

High Energy Astrophysical Phenomena · Physics 2015-06-18 Yi Xing , Zhongxiang Wang

We report on a multi-wavelength study of the unclassified X-ray source CXOU J110926.4-650224 (J1109). We identified the optical counterpart as a blue star with a magnitude of $\sim$20.1 (3300-10500 $\require{mediawiki-texvc} \AA$). The…

The gamma-ray binary 1FGL J1018.6-5856 consists of an O6V((f)) type star and an unknown compact object, and shows orbitally modulated emission from radio to very high energy gamma rays. The X-ray light curve shows a maximum around the same…

High Energy Astrophysical Phenomena · Physics 2022-07-06 B. van Soelen , S. Mc Keague , D. Malyshev , M. Chernyakova , N. Komin , N. Matchett , I. M. Monageng

The Fermi catalogue contains about 2000 unassociated $\gamma$-ray sources. Some of them were recently identified as pulsars, including so called redbacks and black widows, which are millisecond pulsars in tight binary systems with non- and…

High Energy Astrophysical Phenomena · Physics 2023-07-06 A. V. Karpova , D. A. Zyuzin , Yu. A. Shibanov , M. R. Gilfanov

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…

High Energy Astrophysical Phenomena · Physics 2025-03-28 K. I. I. Koljonen , M. Linares , J. C. A. Miller-Jones

Transitional millisecond pulsars are millisecond pulsars that switch between a rotation-powered millisecond pulsar state and an accretion-powered X-ray binary state, and are thought to be an evolutionary stage between neutron star low-mass…

The Fermi source 4FGL J1848.7-0129 has been historically related to the globular cluster GLIMPSE-C01 since its very first detection. Although this association is widely accepted, as it appears in the most recent Fermi catalog, it deserves…

High Energy Astrophysical Phenomena · Physics 2022-12-07 Pedro L. Luque-Escamilla , Josep Martí , Enrique Mestre , Jorge A. Combi , Juan F. Albacete-Colombo

Very faint X-ray transients (VFXTs) are a group of X-ray binaries with low luminosities, the peak X-ray luminosities during their outbursts being only 10$^{34}$--10$^{36}$ erg\,s$^{-1}$. Using the $\gamma$-ray data obtained with the Large…

High Energy Astrophysical Phenomena · Physics 2018-09-19 Gege Wang , Zhongxiang Wang

The Fermi source 2FGL~J0523.3$-$2530 has recently been identified as a candidate millisecond pulsar binary with an orbital period of 16.5 hrs. We have carried out detailed studies of the source's emission properties by analyzing data taken…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Yi Xing , Zhongxiang Wang , C. -Y. Ng

3FGL J1544.6-1125 is a candidate transitional millisecond pulsar (tMSP). Similar to the well-established tMSPs - PSR J1023+0038, IGR J18245-2452, and XSS J12270-4859 -- 3FGL J1544.6-1125 shows $\gamma$-ray emission and discrete X-ray "low"…

We report the discovery of a new black-widow millisecond pulsar, PSR J1544-2555, associated with the Fermi-LAT source 4FGL J1544.2-2554. Optical, radio, and gamma-ray observations confirmed its nature as a compact spider binary system.…

We present the study of multi-wavelength observations of an unidentified Fermi Large Area Telescope (LAT) source, 4FGL J1910.7-5320, a new candidate redback millisecond pulsar binary. In the 4FGL 95% error region of 4FGL J1910.7-5320, we…

A rare group of high mass X-ray binaries (HMXBs) are known that also exhibit MeV, GeV, and/or TeV emission ("gamma-ray binaries"). Expanding the sample of gamma-ray binaries and identifying unknown Fermi sources are currently of great…

High Energy Astrophysical Phenomena · Physics 2013-05-14 M. Virginia McSwain , Masha Chernyakova , Denis Malishev , Michael De Becker , Stephen Williams

We present a comprehensive study of the flaring mode of the transitional millisecond pulsar (tMSP) PSR J1023+0038 during its X-ray sub-luminous state, using strictly simultaneous X-ray, UV, optical, and radio observations. The X-ray flares…

The X-ray source XSS J12270-4859 has been first suggested to be a magnetic cataclysmic variable of Intermediate Polar type on the basis of its optical spectrum and a possible 860 s X-ray periodicity. However further X-ray observations by…

Space Physics · Physics 2012-02-14 J. M. Bonnet-Bidaud , D. de Martino , M. Mouchet , M. Falanga , T. Belloni , N. Masetti , K. Mukai , G. Matt

We have searched for millisecond pulsars (MSPs) in two globular clusters detected by the Fermi Large Area Telescope. These clusters contained no known MSPs prior to their detections in gamma rays. The discovery of gamma ray emission from…

High Energy Astrophysical Phenomena · Physics 2011-11-03 Megan E. DeCesar , Scott M. Ransom , Paul S. Ray