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Revisiting the ultraluminous supersoft source in M 101: an optically thick outflow model
Online Contents | 2016|Contributors: Soria, Roberto -
Spectra of black hole accretion models of ultraluminous X-ray sources
Online Contents|Contributors: Soria, Roberto -
THE BIRTH OF AN ULTRALUMINOUS X-RAY SOURCE IN M83Based on observations made with NASA's Chandra X-Ray Observatory, the NASA/ESA Hubble Space Telescope (HST), Swift, the 6.5 m Magellan Telescopes located at Las Campanas Observatory, and the Gemini Observatory. NASA's Chandra Observatory is operated by Smithsonian Astrophysical Observatory under contract NAS83060, and the data were obtained through program GO1-12115. The HST observations were obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contract NAS 5-26555. The new HST observations were obtained through programs GO-12513 and GO-12683. Data in the HST archive from program GO-11360 were also used. The ground-based observations were obtained from the Magellan I Telescope at the Las Campanas Observatory and from the Gemini South Telescope of the Gemini Observatory, both awarded through NOAO, which is operated by Association of Universities for Research i
Online Contents | 2012| -
THE FADING OF TWO TRANSIENT ULTRALUMINOUS X-RAY SOURCES TO BELOW THE STELLAR MASS EDDINGTON LIMIT
Online Contents | 2013|Contributors: Soria, Roberto -
The nature of the companion star in Circinus X-1
Online Contents | 2015|Contributors: Soria, Roberto -
The star-forming environment of an ultraluminous X-ray source in NGC4559: an optical study
Online Contents | 2005| -
ULTRALUMINOUS X-RAY SOURCE CORRELATIONS WITH STAR-FORMING REGIONS
Online Contents | 2009|Contributors: Soria, Roberto -
ULTRALUMINOUS X-RAY SOURCE CORRELATIONS WITH STAR-FORMING REGIONS
Online Contents | 2009|Contributors: Soria, Roberto
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