Black holes, gravitational waves and fundamental physics: a roadmap

L Barack, V Cardoso, S Nissanke… - … and quantum gravity, 2019 - iopscience.iop.org
AIM, UMR 7158, CEA/DRF, CNRS, Université Paris Diderot, Irfu/Service d'Astrophysique,
Centre de Saclay, FR-91191 Gif-sur-Yvette, France

[HTML][HTML] Advances in understanding high-mass X-ray binaries with INTEGRALand future directions

P Kretschmar, F Fürst, L Sidoli, E Bozzo… - New Astronomy …, 2019 - Elsevier
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 …

Periodic activity from a fast radio burst source

Nature, 2020 - nature.com
Fast radio bursts (FRBs) are bright, millisecond-duration radio transients originating from
sources at extragalactic distances, the origin of which is unknown. Some FRB sources emit …

Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+ 4127/MT91 213 on its approach to periastron

WCG Ho, CY Ng, AG Lyne, BW Stappers… - Monthly Notices of …, 2017 - academic.oup.com
The radio and gamma-ray pulsar PSR J2032+ 4127 was recently found to be in a decades-
long orbit with the Be star MT91 213, with the pulsar moving rapidly towards periastron. This …

The geometric distance and binary orbit of PSR B1259–63

JCA Miller-Jones, AT Deller… - Monthly Notices of …, 2018 - academic.oup.com
The pulsar/massive star binary system PSR B1259− 63/LS 2883 is one of the best-studied
gamma-ray binaries, a class of systems whose bright gamma-ray flaring can provide …

NuSTAR observation of LS 5039

I Volkov, O Kargaltsev, G Younes, J Hare… - The Astrophysical …, 2021 - iopscience.iop.org
LS 5039 is a high-mass γ-ray binary hosting a compact object of unknown type. NuSTAR
observed LS 5039 during the entire 3.9-day binary period. We performed a periodic signal …

[HTML][HTML] Multi-wavelength properties of the 2021 Periastron passage of PSR B1259-63

M Chernyakova, D Malyshev, B van Soelen… - Universe, 2021 - mdpi.com
PSR B1259-63 is a gamma-ray binary system hosting a radio pulsar orbiting around a O9.
5Ve star, LS 2883, with a period of∼ 3.4 years. The interaction of the pulsar wind with the LS …

Introduction to multi-messenger astronomy

A Neronov - Journal of Physics: Conference Series, 2019 - iopscience.iop.org
The new field of multi-messenger astronomy aims at the study of astronomical sources using
different types of" messenger" particles: photons, neutrinos, cosmic rays and gravitational …

Overview of non-transient γ-ray binaries and prospects for the Cherenkov Telescope Array

M Chernyakova, D Malyshev, A Paizis… - Astronomy & …, 2019 - aanda.org
Aims. Despite recent progress in the field, there are still many open questions regarding γ-
ray binaries. In this paper we provide an overview of non-transient γ-ray binaries and …

HESS and Fermi-LAT observations of PSR B1259–63/LS 2883 during its 2014 and 2017 periastron passages

H Abdalla, R Adam, F Aharonian, FA Benkhali… - Astronomy & …, 2020 - aanda.org
Context. PSR B1259–63/LS 2883 is a gamma-ray binary system consisting of a pulsar in an
eccentric orbit around a bright Oe stellar-type companion star that features a dense …