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 …

Abstract The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Project led by
the Italian National Institute for Astrophysics (INAF) is developing and will deploy at the …

Although celestial sources emitting in the few tens of GeV up to a few TeV are being
investigated by imaging atmospheric Čerenkov telescope arrays such as HESS, MAGIC …

Abstract The ASTRI (Astrofisica con Specchi a Tecnologia Replicante Italiana) Mini-Array
will be composed of nine imaging atmospheric Cherenkov telescopes at the Observatorio …

ABSTRACT PSR B1259-63 is a gamma-ray binary system hosting a radio pulsar orbiting
around an O9. 5Ve star, LS 2883, with a period of∼ 3.4 yr. The interaction of the pulsar wind …

Black hole and neutron star environments often comprise collisionless plasmas immersed in
strong magnetic fields and intense baths of low-frequency radiation. In such conditions …

ABSTRACT HESS J1832− 093 is a member of the rare class of gamma-ray binaries, as
recently confirmed by the detection of orbitally modulated X-ray and gamma-ray emission …

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray
imaging (< 1 0 ″FWHM) and broad spectral coverage (0.2–80 keV) with an effective area …

Context. Colliding wind binaries are massive systems featuring strong, interacting stellar
winds which may act as particle accelerators. Therefore, such binaries are good candidates …

ABSTRACT PSR B1259-63 is a gamma-ray binary system with a radio pulsar orbiting an O9.
5Ve star, LS 2883, with a period of yr. Close to the periastron the system is detected at all …