Sökning: id:"swepub:oai:DiVA.org:kth-299620" > The evolution of ra...
Fältnamn | Indikatorer | Metadata |
---|---|---|
000 | 05376naa a2200589 4500 | |
001 | oai:DiVA.org:kth-299620 | |
003 | SwePub | |
008 | 210813s2021 | |||||||||||000 ||eng| | |
009 | oai:DiVA.org:su-196983 | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2996202 URI |
024 | 7 | a https://doi.org/10.1093/mnras/stab15312 DOI |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1969832 URI |
040 | a (SwePub)kthd (SwePub)su | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a ref2 swepub-contenttype |
072 | 7 | a art2 swepub-publicationtype |
100 | 1 | a Paice, J. A.u Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England.;Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India.4 aut |
245 | 1 0 | a The evolution of rapid optical/X-ray timing correlations in the initial hard state of MAXIJ1820+070 |
264 | c 2021-05-27 | |
264 | 1 | b Oxford University Press (OUP),c 2021 |
338 | a print2 rdacarrier | |
500 | a QC 20220413 | |
520 | a We report on a multiepoch campaign of rapid optical/X-ray timing observations of the superbright 2018 outburst of MAXIJ1820+070, a black hole low-mass X-ray binary system. The observations spanned 80 d in the initial hard state and were taken with NTT/ULTRACAM and GTC/HiPERCAM in the optical (u(s)g(s)r(s)i(s)z(s) filters at time resolutions of 8-300Hz) and with ISS/NICER in X-rays. We find (i) a growing anticorrelation between the optical and X-ray light curves, (ii) a steady, positive correlation at an optical lag of similar to 0.2s (with a longer lag at longer wavelengths) present in all epochs, and (iii) a curious positive correlation at negative optical lags in the last, X-ray softest epoch, with longer wavelengths showing a greater correlation and a more negative lag. To explain these, we postulate the possible existence of two synchrotron-emitting components - a compact jet and a hot flow. In our model, the significance of the jet decreases over the outburst, while the hot flow remains static (thus, relatively, increasing in significance). We also discuss a previously discovered quasi-periodic oscillation and note how it creates coherent optical time lags, stronger at longer wavelengths, during at least two epochs. | |
650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
653 | a accretion | |
653 | a accretion discs | |
653 | a X-rays: binaries | |
653 | a X-rays: individual: MAXIJ1820+070 | |
653 | a black holes | |
700 | 1 | a Gandhi, P.u Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England.4 aut |
700 | 1 | a Shahbaz, T.u Inst Astrofis Canarias IAC, E-38205 San Cristobal la Laguna, Tenerife, Spain.;Univ La Laguna ULL, Dept Astrofis, E-38206 San Cristobal la Laguna, Tenerife, Spain.4 aut |
700 | 1 | a Veledina, Alexandrau Stockholms universitet,KTH,Nordic Institute for Theoretical Physics NORDITA,Univ Turku, Dept Phys & Astron, FI-20014 Turku, Finland.;Stockholm Univ, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden.,Nordiska institutet för teoretisk fysik (Nordita),University of Turku, Finland4 aut0 (Swepub:su)avele |
700 | 1 | a Malzac, J.u IRAP Univ Toulouse, CNES, UPS, CNRS, F-31400 Toulouse, France.4 aut |
700 | 1 | a Buckley, D. A. H.u South African Astron Observ, Observ Rd, ZA-7925 Cape Town, South Africa.;Univ Cape Town, Dept Astron, Private Bag X3, ZA-7701 Rondebosch, South Africa.4 aut |
700 | 1 | a Charles, P. A.u Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England.4 aut |
700 | 1 | a Rajwade, K.u Univ Manchester, Dept Phys & Astron, Oxford Rd, Manchester M13 9PL, Lancs, England.4 aut |
700 | 1 | a Dhillon, V. S.u Inst Astrofis Canarias IAC, E-38205 San Cristobal la Laguna, Tenerife, Spain.;Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England.4 aut |
700 | 1 | a Littlefair, S. P.u Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England.4 aut |
700 | 1 | a Marsh, T. R.u Univ Warwick, Dept Phys, Astron & Astrophys Grp, Gibbet Hill Rd, Coventry CV4 7AL, W Midlands, England.4 aut |
700 | 1 | a Uttley, P.u Univ Amsterdam, Astron Inst Anton Pannekoek, Sci Pk 904, NL-1098 XH Amsterdam, Netherlands.4 aut |
700 | 1 | a Vincentelli, F. M.u Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England.4 aut |
700 | 1 | a Misra, R.u Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India.4 aut |
710 | 2 | a Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England.;Interuniv Ctr Astron & Astrophys, Pune 411007, Maharashtra, India.b Univ Southampton, Dept Phys & Astron, Southampton SO17 1BJ, Hants, England.4 org |
773 | 0 | t Monthly notices of the Royal Astronomical Societyd : Oxford University Press (OUP)g 505:3, s. 3452-3469q 505:3<3452-3469x 0035-8711x 1365-2966 |
856 | 4 | u https://arxiv.org/pdf/2105.11769.pdf |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-299620 |
856 | 4 8 | u https://doi.org/10.1093/mnras/stab1531 |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-196983 |
Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.