The Astrophysical Journal · 2003 · 14 citations · 21 references
Natural SciencesAstronomyPhysicsAstrophysicsObservational AstronomyX-ray AstronomyExtragalactic X-ray SourcesX-ray Source CatalogsPower-law ModelSoft X-ray AstronomySoft X-ray BackgroundSoft X-ray SpectroscopySpectral Shape AnalysisUltra-luminous X-ray SourcesUltraluminous X-ray Sources
We report the discovery of a new ultraluminous X-ray source (ULX) in the nearby galaxy NGC 4244 from Chandra archival data. The source, 1WGAJ1216.9+3743, is one of the least luminous and softest ULXs discovered so far. Its X-ray spectrum is the best available for a representative of the soft ULXs, a class of sources recently discovered by Chandra and XMM-Newton. 1WGAJ1216.9+3742 appears point-like in the Chandra image and has a complex spectral shape: a multicolor disk model, suitable for brighter ULXs, is inadequate for this source. 1WGAJ1216.9+3743 spectrum is heavily absorbed (NH ~ (1-4)E21 cm^-2),and very soft. The best-fit power-law model gives a photon index ~ 5 and implies a luminosity L(0.5-10 keV) ~ 1E39 erg/s. A comparison with previous detections shows that, despite the variability displayed by the source during the Chandra observation, 1WGAJ1216.9+3743 count rate, spectral shape and absorption are practically unchange over a 9-year period. We performed also deep optical imaging of the field containing the X-ray source, and found a possible R ~ 23.7 counterpart.
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G. Fabbiano · Annual Review of Astronomy and Astrophysics · 1989 · 755 citations
Ultraluminous X-Ray Sources in External Galaxies
A. R. King, M. B. Davies, M. J. Ward et al. · The Astrophysical Journal · 2001 · 730 citations · Full text
Natural Sciences, Astronomy, Physics +17