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dc.contributor.authorLopez-Navas, E.
dc.contributor.authorDegenaar, N.
dc.contributor.authorParikh, A. S.
dc.contributor.authorSantisteban, J. V. Hernandez
dc.contributor.authorvan den Eijnden, J.
dc.identifier.citationLopez-Navas , E , Degenaar , N , Parikh , A S , Santisteban , J V H & van den Eijnden , J 2020 , ' The connection between the UV/optical and X-ray emission in the neutron star low-mass X-ray binary Aql X-1 ' , Monthly Notices of the Royal Astronomical Society , vol. 493 , no. 1 , pp. 940-951 .
dc.identifier.otherORCID: /0000-0002-6733-5556/work/71221721
dc.descriptionEL-N gratefully acknowledges support from an ‘ERASMUS+ for traineeship’ grant, and is thankful for the hospitality of the Anton Pannekoek Institute, where most of this work was carried out. ND, ASP, JVHS, and JvdE were supported by a Vidi grant from the Netherlands Organisation for Scientific Research (NWO), awarded to ND. JVHS acknowledges support from a Science and Technology Facilities Council (STFC) grant ST/R000824/1.en
dc.description.abstractAccreting neutron stars and black holes in low-mass X-ray binaries (LMXBs) radiate across the electromagnetic spectrum. Linking the emission produced at different wavelengths can provide valuable information about the accretion process and any associated outflows. In this work, we study simultaneous X-ray and ultraviolet (UV)/optical observations of the neutron star LMXB Aql X-1, obtained with the Neil Gehrels Swift Observatory during its 2013, 2014, and 2016 accretion outbursts. We find that the UV/optical and X-ray emission are strongly correlated during all three outbursts. For the 2013 and 2014 episodes, which had the best Swift sampling, we find that the correlation between the UV/optical and X-ray fluxes is significantly steeper during the decay (soft state) of the outburst than during the rise (hard-to-soft state). We observe a UV/optical hysteresis behaviour that is likely linked to the commonly known X-ray spectral hysteresis pattern. For the decays of the three outbursts, we obtain a correlation index that cannot be directly explained by any single model. We suspect that this is a result of multiple emission processes contributing to the UV/optical emission, but we discuss alternative explanations. Based on these correlations, we discuss which mechanisms are likely dominating the UV/optical emission of Aql X-1.
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.subjectAccretion, accretion discsen
dc.subjectStars: neutronen
dc.subjectX-rays: binariesen
dc.subjectX-rays: individual: (Aql X-1)en
dc.subjectQB Astronomyen
dc.titleThe connection between the UV/optical and X-ray emission in the neutron star low-mass X-ray binary Aql X-1en
dc.typeJournal articleen
dc.contributor.sponsorScience & Technology Facilities Councilen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.description.statusPeer revieweden

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