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

Por favor, use este identificador para citar o enlazar este ítem: http://hdl.handle.net/10045/109660
Información del item - Informació de l'item - Item information
Título: Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions
Autor/es: 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. | Bissinger né Kühnel, Matthias | Blay, Pere | Caballero, Isabel | Coe, Malcolm J. | Domingo, Albert | Doroshenko, Victor | Ducci, Lorenzo | Falanga, Maurizio | Grebenev, Sergei A. | Grinberg, Victoria | Hemphill, Paul | Kreykenbohm, Ingo | Kreykenbohm né Fritz, Sonja | 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. | Torrejon, Jose M. | Torres, Diego F. | Walter, Roland | Wilms, Jörn | Wilson-Hodge, Colleen A. | Zhang, Shu
Grupo/s de investigación o GITE: Astrofísica Estelar (AE) | Astronomía y Astrofísica
Centro, Departamento o Servicio: Universidad de Alicante. Departamento de Física Aplicada | Universidad de Alicante. Departamento de Física, Ingeniería de Sistemas y Teoría de la Señal | Universidad de Alicante. Instituto Universitario de Física Aplicada a las Ciencias y las Tecnologías
Palabras clave: X-rays: binaries | Accretion | Stars: neutron | Pulsars: general | Gamma rays: observations | INTEGRAL observatory
Área/s de conocimiento: Astronomía y Astrofísica | Física Aplicada
Fecha de publicación: 9-sep-2020
Editor: Elsevier
Cita bibliográfica: New Astronomy Reviews. 2019, 86: 101546. https://doi.org/10.1016/j.newar.2020.101546
Resumen: 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.
Patrocinador/es: The INTEGRALteams in the participating countries acknowledge the continuous support from their space agencies and funding organizations: the Italian Space Agency ASI (via different agreements including the latest one, 2019-35HH, and the ASIINAF agreement 2017-14-H.0), the French Centre national d’études spatiales (CNES), the Russian Foundation for Basic Research (KP, 19-02-00790), the Russian Science Foundation (ST, VD, AL; 19-12-00423), the Spanish State Research Agency (via different grants including ESP2017-85691-P, ESP2017-87676-C5-1-R and Unidad de Excelencia María de Maeztu – CAB MDM-2017-0737). IN is partially supported by the Spanish Government under grant PGC2018-093741-B-C21/C22 (MICIU/AEI/FEDER, UE). LD acknowledges grant 50 OG 1902.
URI: http://hdl.handle.net/10045/109660
ISSN: 1387-6473 (Print) | 1872-9630 (Online)
DOI: 10.1016/j.newar.2020.101546
Idioma: eng
Tipo: info:eu-repo/semantics/article
Derechos: © 2020 Published by Elsevier B.V.
Revisión científica: si
Versión del editor: https://doi.org/10.1016/j.newar.2020.101546
Aparece en las colecciones:INV - Astrofísica Estelar - Artículos de Revistas
INV - Astronomía y Astrofísica - Artículos de Revistas

Archivos en este ítem:
Archivos en este ítem:
Archivo Descripción TamañoFormato 
ThumbnailKretschmar_etal_2020_NewAstronomyRev_final.pdfVersión final (acceso restringido)2,75 MBAdobe PDFAbrir    Solicitar una copia
ThumbnailKretschmar_etal_2020_NewAstronomyRev_preprint.pdfPreprint (acceso abierto)9,79 MBAdobe PDFAbrir Vista previa


Todos los documentos en RUA están protegidos por derechos de autor. Algunos derechos reservados.