Discovery and Interpretation of an X-Ray Period in the Galactic Center Source CXOGC J174536.1–285638
暂无分享,去创建一个
[1] H. Murakami,et al. Suzaku X-Ray Spectroscopy of a Peculiar Hot Star in the Galactic Center Region , 2007, 0712.0280.
[2] S. Smartt,et al. The VLT-FLAMES survey of massive stars: wind properties and evolution of hot massive stars in the Large Magellanic Cloud , 2007, 0704.1113.
[3] Nicolas Produit,et al. A description of sources detected by INTEGRAL during the first 4 years of observations , 2007, astro-ph/0703043.
[4] L. Titarchuk,et al. Power Spectra of Black Holes and Neutron Stars as a Probe of Hydrodynamic Structure of the Source: Diffusion Theory and Its Application to Cygnus X-1 and Cygnus X-2 X-Ray Observations , 2006, astro-ph/0612675.
[5] P. Crowther,et al. Physical Properties of Wolf-Rayet Stars , 2006, astro-ph/0610356.
[6] M. Schurch,et al. A search for counterparts to massive X-ray binaries using photometric catalogues ,⋆ , 2006, astro-ph/0610006.
[7] M. Irwin,et al. The UKIRT Infrared Deep Sky Survey (UKIDSS) , 2006, astro-ph/0604426.
[8] A. Pollock,et al. XMM-Newton observations of the massive colliding wind binary and non-thermal radio emitter Cyg OB2#8A [O6If+O5.5III(f)] , 2006 .
[9] S. Eikenberry,et al. Identification of the Infrared Counterpart to a Newly Discovered X-Ray Source in the Galactic Center , 2006, astro-ph/0607147.
[10] T. Oosterbroek,et al. Unveiling the nature of the highly absorbed X-ray source SAX J1748.2-2808 with XMM-Newton , 2006, astro-ph/0606307.
[11] W. Lewin,et al. Compact stellar X-ray sources , 2006 .
[12] J. Tomsick,et al. Identifications of Four INTEGRAL Sources in the Galactic Plane via Chandra Localizations , 2006, astro-ph/0603810.
[13] S. Farrell,et al. Super-orbital periods in X-ray binaries , 2006 .
[14] N. Gehrels,et al. Swift, INTEGRAL, RXTE, and Spitzer Reveal IGR J16283–4838 , 2005, astro-ph/0506170.
[15] S. Chaty,et al. The Optical/Near-Infrared Counterpart of the INTEGRAL Obscured Source IGR J16318–4848: An sgB[e] in a High-Mass X-Ray Binary? , 2004, astro-ph/0408407.
[16] John T. Rayner,et al. Spextool: A Spectral Extraction Package for SpeX, a 0.8–5.5 Micron Cross‐Dispersed Spectrograph , 2004 .
[17] E. Feigelson,et al. The Spectra and Variability of X-Ray Sources in a Deep Chandra Observation of the Galactic Center , 2004, astro-ph/0403463.
[18] H. Sana,et al. A phase-resolved XMM–Newton campaign on the colliding-wind binary HD 152248 , 2004, astro-ph/0402412.
[19] MIT,et al. Diffuse X-Ray Emission in a Deep Chandra Image of the Galactic Center , 2004, astro-ph/0402087.
[20] John T. Rayner,et al. SpeX: A Medium‐Resolution 0.8–5.5 Micron Spectrograph and Imager for the NASA Infrared Telescope Facility , 2003 .
[21] J. Clark,et al. Near IR spectroscopy of the X-ray binary Circinus X-1 , 2003 .
[22] W. N. Brandt,et al. A Deep Chandra Catalog of X-Ray Point Sources toward the Galactic Center , 2003, astro-ph/0301371.
[23] H Germany,et al. A Method of Correcting Near‐Infrared Spectra for Telluric Absorption , 2002, astro-ph/0211255.
[24] M. Coe,et al. Long-term properties of accretion discs in X-ray binaries – I. The variable third period in SMC X-1 , 2002, astro-ph/0210241.
[25] L. Girardi,et al. Theoretical isochrones in several photometric systems I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets , 2002, astro-ph/0205080.
[26] J. Lee,et al. The First High-Resolution X-Ray Spectrum of Cygnus X-1: Soft X-Ray Ionization and Absorption , 2001, astro-ph/0109236.
[27] Andrew King,et al. Accretion Power in Astrophysics: Contents , 2002 .
[28] M. Shara,et al. Spatially Resolved STIS Spectra of WR + OB Binaries with Colliding Winds , 2001, astro-ph/0111496.
[29] Karel A. van der Hucht,et al. The VIIth catalogue of galactic Wolf–Rayet stars , 2001 .
[30] G. Dubus,et al. Precessing warped accretion discs in X‐ray binaries , 2000, astro-ph/0009264.
[31] S. Kitamoto,et al. Changes in the Long-Term Intensity Variations in Cygnus X-2 and LMC X-3 , 2000, astro-ph/0002219.
[32] J. Fabregat,et al. The Be Phenomenon in Early-Type Stars , 2000 .
[33] John Scott Drilling,et al. in Allen''''s Astrophysical Quantities , 2000 .
[34] Myron A Smith. The Be Phenomenon in Early‐Type Stars: IAU Colloquium 175 , 1999 .
[35] D. Vanbeveren,et al. The WR and O-type star population predicted by massive star evolutionary synthesis , 1998 .
[36] K. Ishibashi,et al. The relationship between two periodicities observed in Eta Carinae , 1998 .
[37] I. McLean,et al. A K-Band Spectral Atlas of Wolf-Rayet Stars , 1997 .
[38] M. Rieke,et al. A spectral atlas of hot, luminous stars at 2 microns , 1996 .
[39] C. Day,et al. Ginga observations of Centaurus X-3 , 1992 .
[40] R. McCray,et al. X-rays from colliding stellar winds , 1990 .
[41] S. Baliunas,et al. A Prescription for period analysis of unevenly sampled time series , 1986 .
[42] D. Raine,et al. Accretion power in astrophysics , 1985 .
[43] Walter H. G. Lewin,et al. X-ray binaries. , 1976 .
[44] H. Friedman. The X-Ray Universe , 1967 .