FIRST HARD X-RAY DETECTION OF THE NON-THERMAL EMISSION AROUND THE ARCHES CLUSTER: MORPHOLOGY AND SPECTRAL STUDIES WITH NuSTAR
暂无分享,去创建一个
D. Stern | N. Barrière | F. Christensen | W. Craig | J. Tomsick | F. Harrison | K. Madsen | F. Bauer | S. Boggs | F. Baganoff | A. Bodaghee | B. Grefenstette | C. Hailey | K. Mori | M. Nynka | Will Zhang | R. Krivonos | Jaesub Hong | D. Stern
[1] R. Terrier,et al. Echoes of multiple outbursts of Sagittarius A⋆ revealed by Chandra , 2013, 1307.3954.
[2] William W. Zhang,et al. THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION , 2013, Astronomical Telescopes and Instrumentation.
[3] A. Decourchelle,et al. Nonthermal X-rays from low-energy cosmic rays: Application to the 6.4 keV line emission from the Arches cluster region , 2012, 1210.2108.
[4] H. Falcke,et al. CHANDRA/HETGS OBSERVATIONS OF THE BRIGHTEST FLARE SEEN FROM Sgr A* , 2012, 1209.6354.
[5] D. J. Walton,et al. EVIDENCE OF LIGHT-BENDING EFFECTS AND ITS IMPLICATION FOR SPECTRAL STATE TRANSITIONS , 2012, 1208.3277.
[6] S. Gillessen,et al. Fe Kα line emission from the Arches cluster region – evidence for ongoing particle bombardment? , 2011, 1104.2039.
[7] R. Wijnands,et al. A four-year baseline Swift study of enigmatic X-ray transients located near the Galactic center , 2010, 1007.0249.
[8] S. Tsygankov,et al. INTEGRAL/IBIS 7-year All-Sky Hard X-ray Survey - I. Image reconstruction , 2010, 1006.2463.
[9] R. Terrier,et al. FADING HARD X-RAY EMISSION FROM THE GALACTIC CENTER MOLECULAR CLOUD Sgr B2 , 2010, 1005.4807.
[10] París,et al. DISCOVERY OF A SUPERLUMINAL Fe K ECHO AT THE GALACTIC CENTER: THE GLORIOUS PAST OF Sgr A* PRESERVED BY MOLECULAR CLOUDS , 2010, 1003.2001.
[11] K. Mitsuda,et al. Line and Continuum Emission from the Galactic Center. III. Origin of 6.4 keV Line Emission from Molecular Clouds in the Galactic Center , 2009, 0905.3075.
[12] Tsuru Takeshi Go,et al. Time Variability of the Neutral Iron Lines from the Sagittarius B2 Region and Its Implication of a Past Outburst of Sagittarius A , 2009 .
[13] R. Genzel,et al. MONITORING STELLAR ORBITS AROUND THE MASSIVE BLACK HOLE IN THE GALACTIC CENTER , 2008, 0810.4674.
[14] M. Tsujimoto,et al. Suzaku Spectroscopic Study of Hard X-Ray Emission in the Arches Cluster , 2006, astro-ph/0611104.
[15] D. Lis,et al. The Origin of Diffuse X-Ray and γ-Ray Emission from the Galactic Center Region: Cosmic-Ray Particles , 2006, astro-ph/0608710.
[16] G. D. Cesare,et al. First broad band study of the mysterious source 1E 1743.1-2843 , 2006, astro-ph/0607388.
[17] Michael A. Nowak,et al. CIAO: Chandra's data analysis system , 2006, SPIE Astronomical Telescopes + Instrumentation.
[18] Cornelia Lang,et al. The interplay between star formation and the nuclear environment of our Galaxy: deep X-ray observations of the Galactic centre Arches and Quintuplet clusters , 2006, astro-ph/0606282.
[19] M. Revnivtsev. Origin Of The Galactic Ridge X-ray Emission: Millions Of Sources , 2006 .
[20] R. Ross,et al. A comprehensive range of X-ray ionized-reflection models , 2005, astro-ph/0501116.
[21] Cambridge,et al. Hard X-ray view of the past activity of Sgr A in a natural Compton mirror , 2004, astro-ph/0408190.
[22] C. Law,et al. X-Ray Observations of Stellar Clusters Near the Galactic Center , 2004, astro-ph/0404544.
[23] R. Sunyaev,et al. A hard X-ray survey of the Galactic-Center region with the IBIS telescope of the INTEGRAL observatory: A catalog of sources , 2004 .
[24] Eugene Serabyn,et al. Massive Stars in the Arches Cluster , 2002, astro-ph/0208145.
[25] Long-term Mir-Kvant observations of the transient X-ray burster KS 1731-260 , 2002 .
[26] A. Cotera,et al. Detection of X-Ray Emission from the Arches Cluster near the Galactic Center , 2001, astro-ph/0108174.
[27] Aneta Siemiginowska,et al. Sherpa: a mission-independent data analysis application , 2001, SPIE Optics + Photonics.
[28] Astrophysics,et al. ASCA Observations of the Sagittarius B2 Cloud: An X-Ray Reflection Nebula , 1999, The Astrophysical Journal.
[29] E. Serabyn,et al. Hubble Space Telescope/NICMOS Observations of Massive Stellar Clusters near the Galactic Center , 1999 .
[30] E. Serabyn,et al. An extraordinary cluster of massive stars near the centre of the Milky Way , 1998, Nature.
[31] R. Sunyaev,et al. EQUIVALENT WIDTH, SHAPE AND PROPER MOTION OF THE IRON FLUORESCENT LINE EMISSION FROM MOLECULAR CLOUDS AS AN INDICATOR OF THE ILLUMINATING SOURCE X-RAY FLUX HISTORY , 1998 .
[32] A. Hornstrup,et al. A Catalog of 203 Galaxy Clusters Serendipitously Detected in the ROSAT PSPC Pointed Observations , 1998, astro-ph/9803099.
[33] W. Forman,et al. Another Collision for the Coma Cluster , 1996, astro-ph/9610151.
[34] Michael G. Burton,et al. The Discovery of Hot Stars near the Galactic Center Thermal Radio Filaments , 1996 .
[35] Yasuo Tanaka,et al. ASCA View of Our Galactic Center: Remains of Past Activities in X-Rays? , 1996 .
[36] C. Jones,et al. Matched Filter Source Detection Applied to the ROSAT PSPC and the Determination of the Number-Flux Relation , 1995 .
[37] Daniel Gerbal,et al. A Wavelet Analysis Search for Substructures in Eleven X-Ray Clusters of Galaxies , 1994 .
[38] Mikhail N. Pavlinsky,et al. The center of the Galaxy in the recent past : a view from Granat , 1993 .
[39] R. Sunyaev,et al. Low-flux hard state of 1E 1740.7-2942 , 1993 .
[40] C. Garmany,et al. On winds and X-rays of O-type stars , 1991 .
[41] G. Skinner,et al. New X-ray transient source KS 1731-260. , 1990 .