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  • Kajava, J. J. E.Univ Turku, Finnish Ctr Astron ESO FINCH, FI-20014 Turku, Finland. (author)

X-ray dips and a complex UV/X-ray cross-correlation function in the black hole candidate MAXI J1820+070

  • Article/chapterEnglish2019

Publisher, publication year, extent ...

  • 2019-06-06
  • OXFORD UNIV PRESS,2019
  • printrdacarrier

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  • LIBRIS-ID:oai:DiVA.org:kth-259435
  • https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-259435URI
  • https://doi.org/10.1093/mnrasl/slz089DOI
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-172971URI

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  • Language:English
  • Summary in:English

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  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • 20190924
  • MAXI J1820+070, a black hole candidate first detected in early 2018 March, was observed by XMM-Newton during the outburst rise. In this letter we report on the spectral and timing analysis of the XMM-Newton X-ray and UV data, as well as contemporaneous X-ray data from the Swift satellite. The X-ray spectrum is well described by a hard thermal Comptonization continuum. The XMM-Newton X-ray light curve shows a pronounced dipping interval, and spectral analysis indicates that it is caused by a moderately ionized partial covering absorber. The XMM-Newton/OM U-filter data do not reveal any signs of the 17 h orbital modulation that was seen later on during the outburst decay. The UV/X-ray cross-correlation function shows a complex shape, with a peak at positive lags of about 4 s and a precognition dip at negative lags, which is absent during the X-ray dipping episode. Such shape could arise if the UV emission comes partially from synchrotron self-Compton emission near the black hole, as well as from reprocessing of the X-rays in the colder accretion disc further out.

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  • Motta, S. E.Univ Oxford, Dept Phys, Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England. (author)
  • Sanna, A.Univ Cagliari, Dipartimento Fis, SP Monserrato Sestu Km 0-7, I-09042 Monserrato, Italy. (author)
  • Veledina, AlexandraStockholms universitet,KTH,Nordic Institute for Theoretical Physics NORDITA,Univ Turku, Dept Phys & Astron, FI-20014 Turku, Finland.;Stockholm Univ, Roslagstultsbacken 23, SE-10691 Stockholm, Sweden.;Russian Acad Sci, Space Res Inst, Profsoyuznaya Str 84-32, Moscow 117997, Russia.,Nordiska institutet för teoretisk fysik (Nordita),University of Turku, Finland; Space Research Institute of the Russian Academy of Sciences, Russia(Swepub:su)avele (author)
  • Del Santo, M.IASF Palermo, Ist Nazl Astrofis, Via U La Malfa 153, I-90146 Palermo, Italy. (author)
  • Segreto, A.IASF Palermo, Ist Nazl Astrofis, Via U La Malfa 153, I-90146 Palermo, Italy. (author)
  • Univ Turku, Finnish Ctr Astron ESO FINCH, FI-20014 Turku, Finland.Univ Oxford, Dept Phys, Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England. (creator_code:org_t)

Related titles

  • In:Monthly notices of the Royal Astronomical Society: OXFORD UNIV PRESS488:1, s. L18-L230035-87111365-29661745-39251745-3933

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