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Investigating ultraluminous X-ray sources through their multiwavelength variability and broadband spectra

Published online by Cambridge University Press:  23 June 2017

Luca Zampieri Open the ORCID record for Luca Zampieri [Opens in a new window] ,
Elena Ambrosi  and
Amid Nayerhoda
Luca Zampieri
Affiliation:
INAF-Astronomical Observatory of Padova Vicolo dell’Osservatorio 5, 35122 Padova, Italy email: luca.zampieri@oapd.inaf.it
Elena Ambrosi
Affiliation:
Department of Physics and Astronomy, University of Padova, Vicolo Osservatorio 3, 35122 Padova, Italy
Amid Nayerhoda
Affiliation:
Department of Physics and Astronomy, University of Padova, Vicolo Osservatorio 3, 35122 Padova, Italy Institute of Nuclear Physics PAN, ul. Radzikowskiego 152, 31-342 Kraków, Poland
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Abstract

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The population of ultraluminous X-ray sources encompasses accreting compact objects with significantly different masses, from black holes of intermediate mass, to black holes of stellar origin, to neutron stars. Investigating these sources will help us answering crucial questions on the distribution of black hole masses and on mass accretion above the Eddington limit in the local Universe, that have potential implications in other astrophysical areas. In order to perform a detailed investigation of ultraluminous X-ray sources, an accurate modeling of their evolution and multiwavelength emission properties is needed. We report some preliminary results of the activities that we are carrying out at present in this area.

Keywords

accretionaccretion disksmethods: numericalX-rays: binaries
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S324: New Frontiers in Black Hole Astrophysics , September 2016 , pp. 31 - 34
Copyright
Copyright © International Astronomical Union 2017 

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