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dc.rights.license© 2020 The Authors. Published by Elsevier B.V.-
dc.contributor.authorKretschmar, P.-
dc.contributor.authorFürst, F.-
dc.contributor.authorSidoli, L.-
dc.contributor.authorBozzo, E.-
dc.contributor.authorAlfonso Garzón, J.-
dc.contributor.authorBodaghee, A.-
dc.contributor.authorChaty, S.-
dc.contributor.authorChernyakova, M.-
dc.contributor.authorFerrigno, C.-
dc.contributor.authorManousakis, A.-
dc.contributor.authorNegueruela, I.-
dc.contributor.authorPostnov, K.-
dc.contributor.authorPaizis, A.-
dc.contributor.authorReig, P.-
dc.contributor.authorRodes Roca, J. J.-
dc.contributor.authorCoe, M. J.-
dc.contributor.authorDomingo, A.-
dc.contributor.authorDoroshenko, V.-
dc.contributor.authorDucci, L.-
dc.contributor.authorFalanga, M.-
dc.contributor.authorGrebenev, S. A.-
dc.contributor.authorGrinberg, V.-
dc.contributor.authorHemphill, P.-
dc.contributor.authorKreykenbohm, I.-
dc.contributor.authorFritz, S. K.-
dc.contributor.authorLi, J.-
dc.contributor.authorLutovinov, A. A.-
dc.contributor.authorMartínez Nuñez, S.-
dc.contributor.authorMas Hesse, J. M.-
dc.contributor.authorMasetti, N.-
dc.contributor.authorMcBride, V. A.-
dc.contributor.authorNeronov, A.-
dc.contributor.authorPottschmidt, K.-
dc.contributor.authorRodríguez, J.-
dc.contributor.authorRomano, P.-
dc.contributor.authorRothschild, R. E.-
dc.contributor.authorSantangelo, A.-
dc.contributor.authorSguera, V.-
dc.contributor.authorStaubert, R.-
dc.contributor.authorTomsick, J. A.-
dc.contributor.authorTorrejón, José Miguel-
dc.contributor.authorTorres, D. F.-
dc.contributor.authorWalter, R.-
dc.contributor.authorWilms, J.-
dc.contributor.authorWilson Hodge, C. A.-
dc.contributor.authorZhang, S.-
dc.contributor.otherUnidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737-
dc.date.accessioned2021-04-14T08:22:27Z-
dc.date.available2021-04-14T08:22:27Z-
dc.date.issued2019-12-13-
dc.identifier.citationNew Astronomy Reviews 86: 101546(2019)es
dc.identifier.issn1387-6473-
dc.identifier.otherhttps://www.sciencedirect.com/science/article/pii/S1387647320300233-
dc.identifier.urihttp://hdl.handle.net/20.500.12666/328-
dc.description.abstractHigh 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.es
dc.description.sponsorshipBased on observations with INTEGRAL, an ESA project with instruments and a science data center funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Spain, and Switzerland), the Czech Republic, and Poland and with the participation of Russia and the USA. 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 ASI-INAF agreement 2017-14-H.0), the French Centre national d'etudes 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 Maria 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.es
dc.language.isoenges
dc.publisherElsevier BVes
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-093741-B-C21/ES/ESTUDIO EMPIRICO MASIVO DE LA EVOLUCION ESTELAR: DESDE LAS PROTOESTRELLAS HASTA LOS PROGENITORES DE SUPERNOVAS POR COLAPSO GRAVITATORIO Y EMISORES DE ONDAS GRAVITACIONALES/-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2017-85691-P/ES/PREPARANDO LA CIENCIA CON ATHENA X-IFU: ESPECTROSCOPIA DE ALTA RESOLUCION DE BINARIAS DE RAYOS X DE ALTA MASA/-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/ESP2017-87676-C5-1-R-
dc.relationinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PGC2018-093741-B-C22/ES/ENTRE NACIMIENTO Y MUERTE: UN ESTUDIO EMPIRICO DE LA EVOLUCION DE LAS ESTRELLAS LUMINOSAS AZULES/-
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.subjectX-rays: binarieses
dc.subjectAccretionses
dc.subjectStars: neutrones
dc.subjectPulsars: generales
dc.subjectGamma rays: observationses
dc.subjectIntegral observatoryes
dc.titleAdvances in Understanding High-Mass X-ray Binaries with INTEGRALand Future Directionses
dc.typeinfo:eu-repo/semantics/articlees
dc.contributor.orcidWilms, J. [0000-0003-2065-5410]-
dc.contributor.orcidSantangelo, A. [0000-0003-4187-9560]-
dc.contributor.orcidGrinberg, V. [0000-0003-2538-0188]-
dc.contributor.orcidSguera, V. [0000-0001-8202-9381]-
dc.contributor.orcidMartínez Núñez, S. [0000-0002-5134-4191]-
dc.contributor.orcidRodes Roca, J. J. [0000-0003-4363-8138]-
dc.identifier.doi10.1016/j.newar.2020.101546-
dc.contributor.funderAgenzia Spaziale Italiana (ASI)-
dc.contributor.funderIstituto Nazionale Astrofisica (INAF)-
dc.contributor.funderRussian Foundation for Basic Research (RFBR)-
dc.contributor.funderAgencia Estatal de Investigación (AEI)-
dc.description.peerreviewedPeer reviewes
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersion-
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess-
dc.type.coarhttp://purl.org/coar/resource_type/c_6501-
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