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LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00004149naa a2200505 4500
001oai:DiVA.org:kth-259435
003SwePub
008190924s2019 | |||||||||||000 ||eng|
009oai:DiVA.org:su-172971
024a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2594352 URI
024a https://doi.org/10.1093/mnrasl/slz0892 DOI
024a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1729712 URI
040 a (SwePub)kthd (SwePub)su
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a art2 swepub-publicationtype
100a Kajava, J. J. E.u Univ Turku, Finnish Ctr Astron ESO FINCH, FI-20014 Turku, Finland.4 aut
2451 0a X-ray dips and a complex UV/X-ray cross-correlation function in the black hole candidate MAXI J1820+070
264 c 2019-06-06
264 1b OXFORD UNIV PRESS,c 2019
338 a print2 rdacarrier
500 a 20190924
520 a 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.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
650 7a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng
653 a accretion
653 a accretion discs
653 a black hole physics
653 a X-rays: binaries
653 a X-rays: individual: MAXI J1820+070
700a Motta, S. E.u Univ Oxford, Dept Phys, Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England.4 aut
700a Sanna, A.u Univ Cagliari, Dipartimento Fis, SP Monserrato Sestu Km 0-7, I-09042 Monserrato, Italy.4 aut
700a Veledina, Alexandrau Stockholms 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, Russia4 aut0 (Swepub:su)avele
700a Del Santo, M.u IASF Palermo, Ist Nazl Astrofis, Via U La Malfa 153, I-90146 Palermo, Italy.4 aut
700a Segreto, A.u IASF Palermo, Ist Nazl Astrofis, Via U La Malfa 153, I-90146 Palermo, Italy.4 aut
710a Univ Turku, Finnish Ctr Astron ESO FINCH, FI-20014 Turku, Finland.b Univ Oxford, Dept Phys, Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England.4 org
773t Monthly notices of the Royal Astronomical Societyd : OXFORD UNIV PRESSg 488:1, s. L18-L23q 488:1<L18-L23x 0035-8711x 1365-2966x 1745-3925x 1745-3933
856u https://doi.org/10.1093/mnrasl/slz089y Fulltext
856u http://arxiv.org/pdf/1906.06519
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-259435
8564 8u https://doi.org/10.1093/mnrasl/slz089
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-172971

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