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Related papers: A Luminous Gamma-ray Binary in the Large Magellani…

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We present a new edition of the catalogue of the low-mass X-ray binaries in the Galaxy and the Magellanic Clouds. The catalogue contains source name(s), coordinates, finding chart, X-ray luminosity, system parameters, and stellar parameters…

Astrophysics · Physics 2008-11-26 Q. Z. Liu , J. van Paradijs , E. P. J. van den Heuvel

The INTEGRAL satellite has revealed a major population of supergiant High Mass X-ray Binaries in our Galaxy, revolutionizing our understanding of binary systems and their evolution. This population, constituted of a compact object orbiting…

High Energy Astrophysical Phenomena · Physics 2010-05-13 Sylvain Chaty

XMM-Newton archival data for the Small Magellanic Cloud have been examined for the presence of previously undetected X-ray pulsars. One such pulsar, with a period of 202 s, is detected. Its position is consistent with an early B star in the…

Astrophysics · Physics 2009-11-10 W. A. Majid , R. C. Lamb , D. J. Macomb

The Large Magellanic Cloud (LMC) currently hosts around 23 high mass X-ray binaries (HMXBs) of which most are Be/X-ray binaries. The LMC XMM-Newton survey provided follow-up observations of previously known X-ray sources that were likely…

High Energy Astrophysical Phenomena · Physics 2017-12-20 N. van Jaarsveld , D. A. H. Buckley , V. A. McBride , F. Haberl , G. Vasilopoulos , C. Maitra , A. Udalski , B. Miszalski

Gamma-ray loud X-ray binaries are binary systems that show non-thermal broadband emission from radio to gamma rays. If the system comprises a massive star and a young non-accreting pulsar, their winds will collide producing broadband…

High Energy Astrophysical Phenomena · Physics 2011-11-23 V. Zabalza , V. Bosch-Ramon , J. M. Paredes

A growing number of early Be stars discovered in X-ray surveys exhibit X-ray luminosities intermediate between those of normal stars and those of most Be/X-ray binaries in quiescence. Their X-ray spectra are also much harder than those of…

High energy gamma-rays have been detected from Cygnus X-3, a system composed of a Wolf-Rayet star and a black hole or neutron star. The gamma-ray emission is linked to the radio emission from the jet launched in the system. The flux is…

High Energy Astrophysical Phenomena · Physics 2015-05-18 G. Dubus , B. Cerutti , G. Henri

Based on XMM-Newton EPIC data of four pointings towards the Small Magellanic Cloud (SMC), results on timing and spectral analyses of 16 known high mass X-ray binaries (HMXBs) and HMXB candidates in the SMC are presented. We confirm the…

Astrophysics · Physics 2009-11-07 Manami Sasaki , Wolfgang Pietsch , Frank Haberl

Based on recent X-ray observations of the Milky Way, Magellanic Clouds and nearby starburst galaxies we study population of high mass X-ray binaries, their connection with ultra-luminous X-ray sources and relation to the star formation.…

Astrophysics · Physics 2009-11-10 M. Gilfanov , H. -J. Grimm , R. Sunyaev

A neutron star low-mass X-ray binary is a binary stellar system with a neutron star and a low-mass companion star rotating around each other. In this system the neutron star accretes mass from the companion, and as this matter falls into…

High Energy Astrophysical Phenomena · Physics 2010-02-25 Sudip Bhattacharyya

Context. The Magellanic Clouds are our nearest star-forming galaxies. While the population of high-mass X-ray binaries (HMXBs) in the Small Magellanic Cloud (SMC) is relatively well studied, our knowledge about the Large Magellanic Cloud…

We have discovered with XMM-Newton an X-ray source in the core of the globular cluster M13, whose X-ray spectral properties suggest that it is a quiescent neutron star X-ray binary. The spectrum can be well fitted with a pure hydrogen…

Astrophysics · Physics 2011-05-23 Bruce Gendre , Didier Barret , Natalie A. Webb

(abridged) We analysed eight XMM-Newton observations toward the Small Magellanic Cloud (SMC), performed between October 2006 and June 2007, to investigate high mass X-ray binary systems. We found new X-ray binary pulsars with periods of 202…

Astrophysics · Physics 2009-11-13 F. Haberl , P. Eger , W. Pietsch

On MJD 56590-1 (2013 Oct 25-26) observations of the Magellanic Clouds by the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) observatory discovered a previously-unreported bright, flaring X-ray source. This source was initially…

High Energy Astrophysical Phenomena · Physics 2015-06-23 M. J. Coe , E. S. Bartlett , A. J. Bird , F. Haberl , J. A. Kennea , V. A. McBride , L. J. Townsend , A. Udalski

Radio continuum emission has been detected from a planetary nebula in the Large Magellanic Cloud: this is the first radio continuum detection for any planetary nebula outside our galaxy. The radio flux density is a factor of two lower than…

Astrophysics · Physics 2007-05-23 Albert A. Zijlstra , Peter A. M. van Hoof , Jessica M. Chapman , Cecile Loup

Recently, IceCube has observed an excess of astrophysical neutrinos from the Galactic plane. Such a signal may indicate the presence of individual sources or a diffuse neutrino flux from the interactions of Galactic, hadronic cosmic rays.…

High Energy Astrophysical Phenomena · Physics 2025-07-10 Alina Kochocki , Dhiti Doddamreddy , Mehr Un Nisa , Steve Sclafani

We present the discovery of radio emission from the Be/X-ray binary A0538-66 with the Australian Square Kilometre Array Pathfinder (ASKAP), and results from a subsequent weekly monitoring campaign with the MeerKAT radio telescope. A0538-66,…

(abridged) We present the first study that combines binary population synthesis in the Galactic disk and detailed evolutionary calculations of low- and intermediate-mass X-ray binaries (L/IMXBs). We show that the formation probability of…

Astrophysics · Physics 2009-11-07 E. Pfahl , S. Rappaport , Ph. Podsiadlowski

We study sky maps and light curves of gamma-ray emission from neutron stars in compact binaries, and in isolation. We briefly review some gamma-ray emission models, and reproduce sky maps from a standard isolated pulsar in the Separatrix…

High Energy Astrophysical Phenomena · Physics 2022-02-18 Néstor Ortiz , Federico Carrasco , Stephen R. Green , Luis Lehner , Steven L. Liebling , John Ryan Westernacher-Schneider

Binary systems are a well-established subclass of gamma-ray sources. The high mass X-ray binary pulsar 1A~0535+262 has been considered to be a possible gamma-ray emitter for a long time, although former gamma-ray searches using…

High Energy Astrophysical Phenomena · Physics 2023-02-22 X. Hou , W. Zhang , D. F. Torres , L. Ji , J. Li