activity
19982026
most citedThe Be/X-ray transient 4U 0115+63/V635 Cas: II. Outburst mechanisms

124 citations · 1.1k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2026

SXP 31.0 -- the 2025 near-Eddington double X-ray outburst after 26 years of quiescence

Malcolm J. Coe, Thomas M. Gaudin, Itumeleng M. Monageng +5

SXP 31.0 is an X-ray source in the Small Magellanic Cloud (SMC) that was first identified as a Be X-ray Binary (BeXRB) system when it went into X-ray outbusrst in 1998. It is now k…

astro-ph.HE2025

Identification of New Candidate Be/X-Ray Binary Systems in the Small Magellanic Cloud via Analysis of S-CUBED Source Catalog

Thomas M. Gaudin, Jamie A. Kennea, Malcolm J. Coe +1

It has long been known that a large population of Be/X-ray Binaries (BeXRBs) exists in the Milky Way's neighboring dwarf galaxy, the Small Magellanic Cloud (SMC), due to a recent p…

astro-ph.HE2024

CXOU J005245.0-722844: Discovery of a Be Star / White Dwarf binary system in the SMC via a very fast, super-Eddington X-ray outburst event

Thomas M. Gaudin, Malcolm J. Coe, Jamie A. Kennea +4

CXOU J005245.0-722844 is an X-ray source in the Small Magellanic Cloud (SMC) that has long been known as a Be/X-ray binary (BeXRB) star, containing an OBe main sequence star and a…

astro-ph.HE2024

Discovery of a Rare Eclipsing Be/X-ray Binary System, Swift J010902.6-723710 = SXP 182

Thomas M. Gaudin, Jamie A. Kennea, Malcolm J. Coe +5

We report on the discovery of Swift J010902.6-723710, a rare eclipsing Be/X-ray Binary system by the Swift SMC Survey (S-CUBED). Swift J010902.6-723710 was discovered via weekly S-…

astro-ph.HE2024

The 2022 super-Eddington outburst of the source SMC X-2

Malcolm J. Coe, Jamie A. Kennea, Itumeleng M. Monageng +5

SMC X-2 exhibits X-ray outburst behaviour that makes it one of the most luminous X-ray sources in the Small Magellanic Cloud. In the last decade it has undergone two such massive o…

astro-ph.HE2020★ 81 cited

Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions

Peter Kretschmar, Felix Fürst, Lara Sidoli +48

High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology,…