Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/44353
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dc.contributor.authorLiu, Z-
dc.contributor.authorO'Brien, PT-
dc.contributor.authorOsborne, JP-
dc.contributor.authorEvans, PA-
dc.contributor.authorPage, KL-
dc.date.accessioned2019-06-11T12:58:16Z-
dc.date.available2019-06-11T12:58:16Z-
dc.date.issued2019-05-02-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2019, 486, pp. 5709–5715en
dc.identifier.urihttps://academic.oup.com/mnras/article/486/4/5709/5484889en
dc.identifier.urihttp://hdl.handle.net/2381/44353-
dc.description.abstractWe report the X-ray data analysis of two transient ultraluminous X-ray sources (ULXs, hereafter X1 and X2) located in the nearby galaxy NGC 7090. While they were not detected in the 2004 XMM-Newton and 2005 Chandra observations, their 0.3-10 keV X-ray luminosities reached $>3\times10^{39}\,\mathrm{erg\,s^{-1}}$ in later XMM-Newton or Swift observations, showing increases in flux by a factor of $>80$ and $>300$ for X1 and X2, respectively. X1 showed indications of spectral variability: at the highest luminosity, its X-ray spectra can be fitted with a powerlaw ($\Gamma=1.55\pm0.15$), or a multicolour disc model with $T_{\mathrm{in}}=2.07^{+0.30}_{-0.23}$ keV; the X-ray spectrum became softer ($\Gamma=2.67^{+0.69}_{-0.64}$), or cooler ($T_\mathrm{in}=0.64^{+0.28}_{-0.17}$ keV) at lower luminosity. No strong evidence for spectral variability was found for X2. Its X-ray spectra can be fitted with a simple powerlaw model ($\Gamma=1.61^{+0.55}_{-0.50}$), or a multicolour disc model ($1.69^{+1.17}_{-0.48}$ keV). A possible optical counterpart for X1 is revealed in HST imaging. No optical variability is found, indicating that the optical radiation may be dominated by the companion star. Future X-ray and optical observations are necessary to determine the true nature of the compact object.en
dc.description.sponsorshipZL thanks the support from the China Scholarship Council. This work is supported by the Strategic Pioneer Program on Space Science, Chinese Academy of Sciences, Grant No. XDA15052100. PTOB acknowledges support from STFC. JPO, PAE, and KLP acknowledge support from the UK Space Agency. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. This work is based on observation obtained with XMM–Newton, an ESA science mission with instruments and contributions directly fund by ESA Member States and NASA, based on observations made with the NASA/ESA Hubble Space Telescope, and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA) The Chandra data are obtained from the Chandra Data Archive. This research has made use of software provided by the Chandra X-ray Center (CXC) in the application packages CIAO.en
dc.language.isoenen
dc.publisherOxford University Press (OUP), Royal Astronomical Societyen
dc.relation.urihttp://arxiv.org/abs/1904.13044v1-
dc.rightsCopyright © 2019, Oxford University Press (OUP), Royal Astronomical Society. Deposited with reference to the publisher’s open access archiving policy. (http://www.rioxx.net/licenses/all-rights-reserved)en
dc.subjectgalaxies: individual: NGC 7090en
dc.subjectX-rays: binariesen
dc.subjectX-rays: individual: NGC 7090 X1en
dc.subjectNGC 7090 X2en
dc.titleX-ray properties of two transient ULX candidates in galaxy NGC 7090en
dc.typeJournal Articleen
dc.identifier.doi10.1093/mnras/stz1194-
dc.identifier.eissn1365-2966-
dc.description.statusPeer-revieweden
dc.description.versionPublisher Versionen
pubs.organisational-group/Organisationen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERINGen
pubs.organisational-group/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomyen
dc.dateaccepted2019-04-26-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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