Different generations of HMXBs: clues about their formation efficiency from Magellanic Clouds studies

28 Dec 2018 Antoniou Vallia Zezas Andreas Drake Jeremy J. Badenes Carles Haberl Frank Hong Jaesub Plucinsky Paul P. Team the SMC XVP Collaboration

Nearby star-forming galaxies offer a unique environment to study the populations of young ($<$100 Myr) accreting binaries. These systems are tracers of past populations of massive stars that heavily affect their immediate environment and parent galaxies... (read more)

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  • HIGH ENERGY ASTROPHYSICAL PHENOMENA