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Analysis of the reflection spectra of MAXI J1535-571 in the hard and intermediate states

Dong, Yanting and Liu, Zhu and Tuo, Youli and Steiner, James F. and Ge, Mingyu and García, Javier A. and Cao, Xinwu (2022) Analysis of the reflection spectra of MAXI J1535-571 in the hard and intermediate states. Monthly Notices of the Royal Astronomical Society, 514 (1). pp. 1422-1432. ISSN 0035-8711. doi:10.1093/mnras/stac1466. https://resolver.caltech.edu/CaltechAUTHORS:20220802-742430000

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Abstract

We report results on the joint-fit of the NuSTAR and HXMT data for the black hole X-ray binary candidate MAXI J1535-571. The observations were obtained in 2017 when the source evolved through the hard, hard-intermediate, and soft-intermediate states over the rising phase of the outburst. After subtracting continuum components, X-ray reflection signatures are clearly showed in those observations. By modelling the relativistic reflection in detail, we find that the inner radius Rin is relatively stable with R_(in) ≲ 1.55R_g during the three states, which implies that the inner radius likely extends to the innermost stable circular orbit even in the bright hard state. When adopting R_(in) = R_(ISCO), the spin parameter is constrained to be 0.985_(-0.004)^(+0.002) at 90 per cent confidence (statistical only). The best-fitting results reveal that the inclination of the inner accretion disc is ∼70–74 deg, which notably conflicts with the apparent orientation of the ballistic jet (≤45 deg). In addition, both the photon index and the electron temperature increase during the transition from hard to soft state. It seems that the corona evolves from dense low-temperature in the low/hard state to tenuous high-temperature after the state transition, which indicates that the state transition is accompanied by the evolution of the coronal properties.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stac1466DOIArticle
https://arxiv.org/abs/2205.12058arXivDiscussion Paper
https://heasarc.gsfc.nasa.gov/docs/archive.htmlRelated ItemNuSTAR data
http://hxmten.ihep.ac.cn/Related ItemHXMT data
ORCID:
AuthorORCID
Dong, Yanting0000-0002-4584-0463
Liu, Zhu0000-0003-3014-8762
Tuo, Youli0000-0003-3127-0110
Steiner, James F.0000-0002-5872-6061
Ge, Mingyu0000-0002-3776-4536
García, Javier A.0000-0003-3828-2448
Cao, Xinwu0000-0002-2355-3498
Additional Information:© 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society. This article is published and distributed under the terms of the Oxford University Press, Standard Journals Publication Model (https://academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model). Received: 14 March 2022. Revision received: 11 May 2022. Accepted: 23 May 2022. Published: 30 May 2022. The authors thank the referee for the helpful comments to improve our manuscript. This work is supported by the NSFC (11773050, 11833007, 12073023), the science research grants from the China Manned Space Project with NO. CMS-CSST-2021-A06. This work used data from the NuSTAR mission, a project led by the California Institute of Technology, managed by the Jet Propulsion Laboratory, and funded by the National Aeronautics and Space Administration. This work also used the data from the Insight-HXMT mission, a project funded by China National Space Administration (CNSA) and the Chinese Academy of Sciences (CAS). The NuSTAR data and software used in this research are provided by the High Energy Astrophysics Science Archive Research Centre (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. DATA AVAILABILITY. Data used in this article are publicly available from the NuSTAR mission (https://heasarc.gsfc.nasa.gov/docs/archive.html) and HXMT mission (http://hxmten.ihep.ac.cn).
Group:Space Radiation Laboratory
Funders:
Funding AgencyGrant Number
National Natural Science Foundation of China11773050
National Natural Science Foundation of China11833007
National Natural Science Foundation of China12073023
China Manned Space ProjectCMS-CSST-2021-A06
NASA/JPL/CaltechUNSPECIFIED
Subject Keywords:accretion, accretion discs, black hole physics, methods: data analysis, X-rays: individual: MAXI J1535-571
Issue or Number:1
DOI:10.1093/mnras/stac1466
Record Number:CaltechAUTHORS:20220802-742430000
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20220802-742430000
Official Citation:Yanting Dong, Zhu Liu, Youli Tuo, James F Steiner, Mingyu Ge, Javier A García, Xinwu Cao, Analysis of the reflection spectra of MAXI J1535-571 in the hard and intermediate states, Monthly Notices of the Royal Astronomical Society, Volume 514, Issue 1, July 2022, Pages 1422–1432, https://doi.org/10.1093/mnras/stac1466
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:116012
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:02 Aug 2022 22:27
Last Modified:02 Aug 2022 22:27

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