An Optical Study of Stellar and Interstellar Environments of Seven Luminous and Ultraluminous X-Ray Sources
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Robert A. Gruendl | R. Gruendl | Q. Wang | C. Chen | Q. Daniel Wang | You-Hua Chu | R. Williams | Caitlin J. Ramsey | Rosa M. Williams | C.-H. Rosie Chen | Y. Chu | You-Hua Chu | Daniel Wang
[1] Denis Foo Kune,et al. Starburst99: Synthesis Models for Galaxies with Active Star Formation , 1999, astro-ph/9902334.
[2] S. Bergh. New Views of the Magellanic Clouds: IAU Symposium 190* , 1998 .
[3] W. Brandt,et al. ROSAT HRI observations of the Local Group galaxies IC 10, NGC 147 and NGC 185 , 1997, astro-ph/9708211.
[4] Q. Wang,et al. Ultraluminous X-ray source 1E 0953.8+6918 (M81 X-9): an intermediate-mass black hole candidate and its environs , 2002, astro-ph/0201230.
[5] D. Westpfahl,et al. HI in M81. I. Large Scale Structure and Spiral Density Waves , 1996 .
[6] Patrick Seitzer,et al. The Optical Counterpart of an Ultraluminous X-Ray Object in M81 , 2002 .
[7] P. T. O'Brien,et al. The identification of an optical counterpart to the super-Eddington X-ray source, NGC 5204 X-1 , 2001 .
[8] J. M. Miller,et al. X-Ray Spectroscopic Evidence for Intermediate-Mass Black Holes: Cool Accretion Disks in Two Ultraluminous X-Ray Sources , 2003 .
[9] L. Zampieri,et al. Optical counterpart of the ultraluminous X-ray source NGC 1313 X-2 , 2004 .
[10] P. Conti,et al. IC 10 - A 'poor cousin' rich in Wolf-Rayet stars , 1992 .
[11] David M. Matonick,et al. Optically Identified Supernova Remnants in the Nearby Spiral Galaxies NGC 5204, NGC 5585, NGC 6946, M81, and M101 , 1997 .
[12] Koji Mukai,et al. The Optical Counterpart of M101 ULX-1 , 2005 .
[13] M. B. Davies,et al. Ultraluminous X-Ray Sources in External Galaxies , 2001 .
[14] Douglas A. Swartz,et al. The Ultraluminous X-Ray Source Population from the Chandra Archive of Galaxies , 2004, astro-ph/0405498.
[16] S. Smartt,et al. Gemini observations of Wolf-Rayet stars in the Local Group starburst galaxy IC 10 , 2003, astro-ph/0302475.
[17] M. Pakull,et al. Detection of an X-ray-ionized nebula around the black hole candidate binary LMC X-l , 1986, Nature.
[18] Y. Chu,et al. X-rays from superbubbles in the Large Magellanic Cloud , 1990 .
[19] Thibault Lejeune,et al. Database of Geneva stellar evolution tracks and isochrones for (UBV) J (RI) C JHKLL'M, HST-WFPC2, Geneva and Washington photometric systems , 2000 .
[20] Mitchell C. Begelman,et al. Super-Eddington Fluxes from Thin Accretion Disks? , 2002, astro-ph/0203030.
[21] Robert Gruendl,et al. A Critical Examination of Hypernova Remnant Candidates in M101. II. NGC 5471B , 2002 .
[22] Aya Kubota,et al. The Nature of Ultraluminous Compact X-Ray Sources in Nearby Spiral Galaxies , 2000, astro-ph/0001009.
[23] A. Treves,et al. VLT Observations of the Ultraluminous X-Ray Source NGC 1313 X-2 , 2005, astro-ph/0510085.
[24] Chandra and Hubble Space Telescope Confirmation of the Luminous and Variable X-Ray Source IC 10 X-1 as a Possible Wolf-Rayet, Black Hole Binary , 2003, astro-ph/0310039.
[25] Patrick Seitzer,et al. The Optical Counterpart of an Ultraluminous X-Ray Source in NGC 5204 , 2004, astro-ph/0501305.
[26] What Produced the Ultraluminous Supernova Remnant in NGC 6946 , 1999, astro-ph/9912003.
[27] B. Miller,et al. The Optical Counterpart to the Extremely Luminous X-Ray Source near Holmberg IX: A Possible Supershell in a Tidal Tail , 1995 .
[28] Q. Wang,et al. XMM-Newton Spectra of Intermediate-Mass Black Hole Candidates: Application of a Monte Carlo Simulated Model , 2004, astro-ph/0403413.
[29] Barry F. Madore,et al. Deviations from the Local Hubble Flow. I. The Tip of the Red Giant Branch as a Distance Indicator , 2002, astro-ph/0204192.
[30] Giuseppina Fabbiano,et al. X Rays From Normal Galaxies , 1989 .
[31] Robin Ciardullo,et al. A Critical Examination of Hypernova Remnant Candidates in M101. I. MF 83 , 2000, astro-ph/0009238.
[32] A. Zezas,et al. ROSAT observations of the dwarf star‐forming galaxy Holmberg II (UGC 4305) , 1999, astro-ph/9903355.
[33] Richard Mushotzky,et al. The star-forming environment of an ultraluminous X-ray source in NGC 4559: an optical study , 2004 .
[34] E. J. A. Meurs,et al. Populations of high energy sources in galaxies , 2006 .
[35] G. Trinchieri,et al. X-ray observations of spiral galaxies. II. Images and spectral parameters of 13 galaxies , 1987 .
[36] van der Thijs Hulst,et al. NEW VIEWS OF THE MAGELLANIC CLOUDS , 1999 .
[37] B. Miller,et al. H II Regions in M81 Group Dwarf Galaxies , 1994 .
[38] Garth D. Illingworth,et al. The Hubble Space Telescope Extragalactic Distance Scale Key Project. 1: The discovery of Cepheids and a new distance to M81 , 1994 .
[39] P. Kaaret,et al. High-resolution imaging of the He II λ4686 emission line nebula associated with the ultraluminous X-ray source in Holmberg II , 2004, astro-ph/0407031.
[40] R. Petre,et al. A BROAD-BAND X-RAY TELESCOPE OBSERVATION OF THE BLACK HOLE CANDIDATE LMC X-1 , 1994 .