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Black holes / Stellar astronomy / Star types / X-ray astronomy / Astrophysics / Ultraluminous X-ray source / Eddington luminosity / Accretion disc / Intermediate-mass black hole / Astronomy / Space / Physics


Draft version March 31, 2015 Preprint typeset using LATEX style emulateapj vNATURE OF THE EXTREME ULTRALUMINOUS X-RAY SOURCES 3 Grzegorz Wiktorowicz1 , Malgorzata Sobolewska2 , Aleksander Sadowski
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Document Date: 2015-03-30 20:33:59


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City

Davies / Cambridge / Warsaw / /

Company

Farrell S. A. / Rappaport S. A. / Medvedev A. S. / R. SA / acc MBH / J. C. & Scott A. E. / /

Country

Poland / United States / /

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Facility

MIT Kavli Institute / Astronomical Observatory / Warsaw University / /

IndustryTerm

e-prints / energy balance / gravitational binding energy / close binary systems / gas flows / massive binary systems / binary systems / volunteer computing / gas circularizing / neutron star systems / /

Organization

Nicolaus Copernicus Astronomical Center / National Science Foundation / International Monetary Fund / MIT Kavli Institute for Astrophysics and Space Research / US Federal Reserve / National Aeronautics and Space Administration / Warsaw University / Center for Gravitational Wave Astronomy / /

Person

Fuerst / Aleksander Sadowski Krzysztof / Gladstone / Rana / V / Walton / Ldon / /

Position

D. J. / King / particular evolutionary model for binary evolution / /

ProvinceOrState

Alabama / Nova Scotia / M. B. / Massachusetts / /

PublishedMedium

Astronomische Nachrichten / /

Technology

radiation / X-RAY / simulation / /

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http /

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