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相关论文: Discovery and analysis of a ULX nebula in NGC 3521

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We report on Chandra observations of the bright ultra-luminous X-ray (ULX) source in NGC3921. Previous XMM observations reported in the literature show the presence of a bright ULX at a 0.5-10 keV luminosity of 2x10^40 erg/s. Our Chandra…

We present optical observations of a ULX in the nearby spiral galaxy IC 342. This variable source has an average X-ray luminosity of some 10^{40} erg/s. At the position of the source there is an ionized nebula (the "Tooth") having huge…

天体物理学 · 物理学 2007-05-23 Fabien Grise , Manfred W. Pakull , Christian Motch

Despite much observational and theoretical effort little is presently known about the nature of the luminous non-nuclear X-ray sources which appear to largely surpass the Eddington limit of a few solar masses. Here we present first results…

天体物理学 · 物理学 2007-05-23 Manfred W. Pakull , Laurent Mirioni

We present the identification and characterization of the optical counterpart to 2XMM J011942.7+032421, one of the most luminous and distant ultra-luminous X-ray sources (ULXs). The counterpart is located near a star forming region in a…

星系天体物理 · 物理学 2015-06-23 C. M. Gutierrez , D. -S. Moon

We present the results of optical panoramic and long-slit spectroscopy of the nebula MF16 associated with the Ultraluminous X-ray Source NGC6946 ULX-1. More than 20 new emission lines are identified in the spectra. Using characteristic line…

天体物理学 · 物理学 2008-09-03 Pavel Abolmasov , S. Fabrika , O. Sholukhova , Taro Kotani

We present the discovery and interpretation of ionized nebulae around two ultraluminous X-ray sources in M 51; both sources share the rare property of showing X-ray eclipses by their companion stars, and are therefore prime targets for…

高能天体物理现象 · 物理学 2018-01-24 R. Urquhart , R. Soria , H. M. Johnston , M. W. Pakull , C. Motch , A. Schwope , J. C. A. Miller-Jones , G. E. Anderson

The emission-line dwarf galaxy NGC 3413 is known to host a bright X-ray source near its optical center. The 0.3-10 keV luminosity of this source is estimated to be approximately 10$^{39}$ erg$s^{-1}$ potentially qualifying it as an…

高能天体物理现象 · 物理学 2018-10-17 E. Sonbas , K. S. Dhuga , E. Göğüş

Optical photometric and spectroscopic data are presented that show an association of an ultraluminous X-ray source in NGC 7331 with a young star cluster of mass 1.1e5 solar masses and age 4.25 Myr. If the ULX is part of the bright stellar…

We present radio through X-ray results of a bright (10^{40} erg/s in the 0.5 to 8.0 keV band) ultraluminous X-ray source (ULX), CXOU J153434.9+151149, in the starburst, interacting pair of galaxies NGC 5953/5954. Chandra image of this ULX…

天体物理学 · 物理学 2009-11-13 Margarita Rosado , Kajal K. Ghosh , Isaura Fuentes-Carrera

We present a study of a peculiar nebula MF16 associated with an Ultraluminous X-ray Source NGC6946 ULX-1. We use integral-field and long-slit spectral data obtained with the 6-m telescope (Russia). The nebula was for a long time considered…

天体物理学 · 物理学 2015-06-24 P. Abolmasov , S. Fabrika , O. Sholukhova

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…

天体物理学 · 物理学 2009-11-07 I. Cagnoni , R. Turolla , A. Treves , J. -S. Huang , D. W. Kim , M. Elvis , A. Celotti

We present optical observations of an ultraluminous X-ray source (ULX) in Holmberg IX, a dwarf galaxy near M81. The ULX has an average X-ray luminosity of some 10^{40} erg/s. It is located in a huge (400pc x 300pc) ionized nebula being much…

天体物理学 · 物理学 2009-11-11 Fabien Grise , Manfred W. Pakull , Christian Motch

Ultra-luminous X-Ray sources are extra-nuclear point sources in external galaxies with $L_X=10^{39}$--$10^{41}$ erg/s and are among the most poorly understood X-ray sources. To help understand their nature, we are trying to identify their…

天体物理学 · 物理学 2009-11-10 Ji-Feng Liu Joel N. Bregman , Patrick Seitzer

We report the detection of radio emission coincident with the ultraluminous X-ray source (ULX) in Holmberg II. The radio emission is diffuse and resolved, covering an area ~60 by 40 pc in extent and well-matched to the recently discovered…

天体物理学 · 物理学 2009-11-10 Neal A. Miller , Richard Mushotzky , Susan Neff

We present optical integral field observations of the H II region containing the ultraluminous X-ray source Holmberg II X-1. We confirm the existence of an X-ray ionized nebula as the counterpart of the source due to the detection of an…

We report the X-ray data analysis of two transient ultraluminous X-ray sources (ULXs, hereafter X1 and X2) located in the nearby galaxy NGC 7090. While they were not detected in the 2004 XMM-Newton and 2005 Chandra observations, their…

高能天体物理现象 · 物理学 2019-05-08 Zhu Liu , P. T. O'Brien , J. P. Osborne , P. A. Evans , K. L. Page

We report the results of a 2-month campaign conducted with the Chandra X-ray observatory to monitor the ultraluminous X-ray source (ULX) NGC 5204 X-1. This was composed of a 50-ks observation, followed by ten 5-ks follow-ups spaced…

天体物理学 · 物理学 2009-11-11 T. P. Roberts , R. E. Kilgard , R. S. Warwick , M. R. Goad , M. J. Ward

To further understand the nature of the optical counterparts associated with Ultraluminous X-Ray sources (ULXs), we obtained far ultraviolet spectra of the reported counterparts to the ULXs in NGC 1313, Holmberg II, NGC 5204, and M81. The…

高能天体物理现象 · 物理学 2012-05-03 Joel N. Bregman , Julie N. Felberg , Patrick J. Seitzer , Jifeng Liu , Martin Kümmel

Ultraluminous X-ray sources (ULXs) are extragalactic X-ray emitters located off-center of their host galaxy and with a luminosity in excess of a few ${10^{39}\text{ erg s}^{-1}}$, if emitted isotropically. The discovery of periodic…

Since their discovery, Ultraluminous X-ray sources (ULXs) have attracted attention due to their combination of extreme luminosities and extra-nuclear locations. However, they are a fairly rare phenomenon, and attempts to investigate the…

高能天体物理现象 · 物理学 2015-05-20 D. J. Walton , J. C. Gladstone , T. P. Roberts , A. C. Fabian
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