Advances in understanding high-mass X-ray binaries with INTEGRAL and Future Directions

作     者：Kretschmar, Peter Fürst, Felix Sidoli, Lara Bozzo, Enrico Alfonso-Garzón, Julia Bodaghee, Arash Chaty, Sylvain Chernyakova, Masha Ferrigno, Carlo Manousakis, Antonios Negueruela, Ignacio Postnov, Konstantin Paizis, Adamantia Reig, Pablo Rodes-Roca, José Joaquín Tsygankov, Sergey Bird, Antony J. né Kühnel, Matthias Bissinger Blay, Pere Caballero, Isabel Coe, Malcolm J. Domingo, Albert Doroshenko, Victor Ducci, Lorenzo Falanga, Maurizio Grebenev, Sergei A. Grinberg, Victoria Hemphill, Paul Kreykenbohm, Ingo née Fritz, Sonja Kreykenbohm Li, Jian Lutovinov, Alexander A. Martínez-Núñez, Silvia Mas-Hesse, J. Miguel Masetti, Nicola McBride, Vanessa A. Neronov, Andrii Pottschmidt, Katja Rodriguez, Jérôme Romano, Patrizia Rothschild, Richard E. Santangelo, Andrea Sguera, Vito Staubert, Rüdiger Tomsick, John A. Torrejón, José Miguel Torres, Diego F. Walter, Roland Wilms, Jörn Wilson-Hodge, Colleen A. Zhang, Shu 

作者机构：E-28692 Spain E-28692 Spain INAF - IASF Istituto di Astrofisica Spaziale e Fisica Cosmica Via A. Corti 12 MilanoI-20133 Italy Department of Astronomy ISDC University of Geneva Chemin d'Ecogia 16 VersoixCH-1290 Switzerland E-28692 Spain Department of Chemistry Physics and Astronomy Georgia College and State University MilledgevilleGA31061 United States AIM CEA CNRS Université Paris-Saclay Université de Paris Gif-sur-YvetteF-91191 France Université de Paris CNRS Astroparticule et Cosmologie ParisF-75006 France School of Physical Sciences and CfAR Dublin City University Dublin 9 Ireland Dublin Institute for Advanced Studies 31 Fitzwilliam Place Dublin 2 Ireland Department of Applied Physics & Astronomy University of Sharjah Sharjah United Arab Emirates  Sharjah United Arab Emirates Department of Applied Physics University of Alicante AlicanteE-03080 Spain Sternberg Astronomical Institute Moscow State University Moscow119234 Russia Kazan Federal University Kazan Russia Institute of Astrophysics Foundation for Research and Technology-Hellas Heraklion Crete71110 Greece University of Crete Physics Department Institute of Theoretical & Computational Physics Heraklion Crete70013 Greece Department of Physics Systems Engineering and Signal Theory University of Alicante AlicanteE-03690 Spain University Institute of Physics Applied to Sciences and Technologies University of Alicante AlicanteE-03690 Spain Department of Physics and Astronomy University of Turku FI-20014 Finland Space Research Institute The Russian Academy of Sciences Profsoyuznaya Str. 84/32 Moscow117997 Russia School of Physics and Astronomy Faculty of Physical Sciences and Engineering University of Southampton SouthamptonSO17 1BJ United Kingdom  Erwin-Rommel-Strae 1 Erlangen91058 Germany Universidad Internacional de Valencia - VIU C/Pintor Sorolla 21 Valencia46002 Spain E-28692 Spain Institut für Astronomie und Astrophysik Universität Tübingen Sand 1 Tübingen72076 Germany  Hallerstrasse 6 BernCH-3012 Switzerland MIT Kavli Institute for Astrophysics and Space Research Massachusetts Institute of Technology CambridgeMA02139 United States Dr. Karl Remeis-Sternwarte Friedrich-Alexander-Universität Erlangen-Nürnberg Sternwartstr. 7 BambergD-96049 Germany Franz-Ludwig-Gymnasium Franz-Ludwig-Strasse 13 Bamberg96047 Germany Deutsches Elektronen Synchrotron DESY ZeuthenD-15738 Germany  SantanderE-39005 Spain INAF - OAS Osservatorio di Astrofisica e Scienza dello Spazio Area della Ricerca del CNR via Gobetti 93/3 BolognaI-40129 Italy Departamento de Ciencias Físicas Universidad Andrés Bello Fernández Concha 700 Las Condes Santiago Chile South African Astronomical Observatory Observatory Road Observatory Cape Town7925 South Africa Inter-University Institute for Data-Intensive Astronomy Department of Astronomy University of Cape Town Private Bag X3 Rondebosch7701 South Africa IAU-Office of Astronomy for Development P.O. Box 9 Observatory7935 South Africa CRESST Department of Physics Center for Space Science and Technology UMBC BaltimoreMD21250 United States NASA Goddard Space Flight Center GreenbeltMD20771 United States INAF - Osservatorio Astronomico di Brera Via E. Bianchi 46 MerateI-23807 Italy Center for Astrophysics and Space Sciences University of California San Diego 9500 Gilman Drive San DiegoCA920093-0424 United States Space Sciences Laboratory University of California 7 Gauss Way BerkeleyCA94720-7450 United States  Campus UAB Carrer de Can Magrans s/n BarcelonaE-08193 Spain  Gran Capità 2-4 BarcelonaE-08034 Spain  BarcelonaE-08010 Spain ST12 Astrophysics Branch NASA Marshall Space Flight Center HuntsvilleAL35812 United States Key Laboratory of Particle Astrophysics Institute of High Energy Physics Chinese Academy of Sciences 19B Yuquan Road Shijingshan District Beijing100049 China 

出 版 物：《arXiv》 (arXiv)

年 卷 期：2020年

核心收录：

主　　题：Galaxies 

摘      要：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, they have attracted the interest of the high energy astrophysical community since the dawn of X-ray Astronomy. In more recent years, they have challenged our comprehension of physical processes in many more energy bands, ranging from the infrared to very high energies. In this review, we provide a broad but concise summary of the physical processes dominating the emission from high mass X-ray binaries across virtually the whole electromagnetic spectrum. These comprise the interaction of stellar winds with the high gravitational and magnetic fields of compact objects, the behaviour of matter under extreme magnetic and gravity conditions, and the perturbation of the massive star evolutionary processes by presence in a binary system. We highlight the role of the INTEGRAL mission in the discovery of many of the most interesting objects in the high mass X-ray binary class and its contribution in reviving the interest for these sources over the past two decades. We show how the INTEGRAL discoveries have not only contributed to significantly increase the number of high mass X-ray binaries known, thus advancing our understanding of the population as a whole, but also have opened new windows of investigation that stimulated the multi-wavelength approach nowadays common in most astrophysical research fields. We conclude the review by providing an overview of future facilities being planned from the X-ray to the very high energy domain that will hopefully help us in finding an answer to the many questions left open after more than 18 years of INTEGRAL scientific observations. Copyright © 2020, The Authors. All rights reserved.