Search Results - "SORIA, Roberto"

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  1. 1

    Spectra of black hole accretion models of ultraluminous X-ray sources by Narayan, Ramesh, Sa̧dowski, Aleksander, Soria, Roberto

    “…Abstract We present general relativistic radiation magnetohydrodynamics simulations of super-Eddington accretion on a 10 M⊙ black hole. We consider a range of…”
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    Journal Article
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    Ultraluminous X-ray sources in the Chandra and XMM-Newton era by Feng, Hua, Soria, Roberto

    Published in New astronomy reviews (01-11-2011)
    “…Ultraluminous X-ray sources (ULXs) are accreting black holes that may contain the missing population of intermediate mass black holes or reflect…”
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    Revisiting the ultraluminous supersoft source in M 101: an optically thick outflow model by Soria, Roberto, Kong, Albert

    “…The M 101 galaxy contains the best-known example of an ultraluminous supersoft source (ULS), dominated by a thermal component at kT ≈ 0.1 keV. The origin of…”
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    On the Short-period Eclipsing High-mass X-Ray Binary in NGC 4214 by Lin, Zikun, Soria, Roberto, Swartz, Douglas A.

    Published in The Astrophysical journal (01-09-2023)
    “…Abstract We present the results of our study of the luminous ( L X ≈ 10 39 erg s −1 ) X-ray binary CXOU J121538.2+361921 in NGC 4214, the high-mass X-ray…”
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    DOES THE INTERMEDIATE-MASS BLACK HOLE IN LEDA 87300 (RGG 118) FOLLOW THE NEAR-QUADRATIC Mbh-Mspheroid RELATION? by Graham, Alister W., Ciambur, Bogdan C., Soria, Roberto

    Published in The Astrophysical journal (17-02-2016)
    “…ABSTRACT The mass scaling relation between supermassive black holes and their host spheroids has previously been described by a quadratic or steeper relation…”
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    A 300-parsec-long jet-inflated bubble around a powerful microquasar in the galaxy NGC 7793 by Pakull, Manfred W, Motch, Christian, Soria, Roberto

    Published in Nature (08-07-2010)
    “…Black-hole accretion states near or above the Eddington luminosity (the point at which radiation force outwards overcomes gravity) are still poorly known…”
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    CG X-1: An Eclipsing Wolf-Rayet ULX in the Circinus Galaxy by Qiu, Yanli, Soria, Roberto, Wang, Song, Wiktorowicz, Grzegorz, Liu, Jifeng, Bai, Yu, Bogomazov, Alexey, Stefano, Rosanne Di, Walton, Dominic J., Xu, Xiaojie

    Published in The Astrophysical journal (20-05-2019)
    “…We investigated the time-variability and spectral properties of the eclipsing X-ray source Circinus Galaxy X-1 (GG X-1), using Chandra, XMM-Newton and ROSAT…”
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    Outbursts of the intermediate-mass black hole HLX-1: a wind-instability scenario by Soria, Roberto, Musaeva, Aina, Wu, Kinwah, Zampieri, Luca, Federle, Sara, Urquhart, Ryan, van der Helm, Edwin, Farrell, Sean

    “…Abstract We model the intermediate-mass black hole HLX-1, using the Hubble Space Telescope, XMM–Newton and Swift. We quantify the relative contributions of a…”
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    Identification of Intermediate-mass Black Hole Candidates among a Sample of Sd Galaxies by Davis, Benjamin L., Graham, Alister W., Soria, Roberto, Jin, Zehao, Karachentsev, Igor D., Karachentseva, Valentina E., D’Onghia, Elena

    Published in The Astrophysical journal (01-08-2024)
    “…Abstract We analyzed images of every northern hemisphere Sd galaxy listed in the Third Reference Catalogue of Bright Galaxies with a relatively face-on…”
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    The SiTian Project by Liu, Jifeng, Soria, Roberto, Wu, Xue-Feng, Wu, Hong, Shang, Zhaohui

    Published in Anais da Academia Brasileira de Ciências (01-01-2021)
    “…SiTian is an ambitious ground-based all-sky optical monitoring project, developed by the Chinese Academy of Sciences. The concept is an integrated network of…”
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  14. 14

    Discovery of two eclipsing X-ray binaries in M 51 by Wang, Song, Soria, Roberto, Urquhart, Ryan, Liu, Jifeng

    “…Abstract We discovered eclipses and dips in two luminous (and highly variable) X-ray sources in M 51. One (CXOM51 J132943.3+471135) is an ultraluminous…”
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    Radio lobes and X-ray hotspots in the microquasar S26 by Soria, Roberto, Pakull, Manfred W., Broderick, Jess W., Corbel, Stephane, Motch, Christian

    “…We have studied the structure and energetics of the powerful microquasar/shock-ionized nebula S26 in NGC 7793, with particular focus on its radio and X-ray…”
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    How rapidly do neutron stars spin at birth? Constraints from archival X-ray observations of extragalactic supernovae by Perna, Rosalba, Soria, Roberto, Pooley, Dave, Stella, Luigi

    “…Traditionally, studies aimed at inferring the distribution of birth periods of neutron stars are based on radio surveys. Here we propose an independent method…”
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    Optical counterpart of HLX-1 during the 2010 outburst by Soria, Roberto, Hakala, Pasi J., Hau, George K. T., Gladstone, Jeanette C., Kong, Albert K. H.

    “…We studied the optical counterpart of the intermediate-mass black hole candidate HLX-1 in ESO 243−49. We used a set of Very Large Telescope imaging…”
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