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20002024
most citedDissecting X-ray-emitting Gas around the Center of our Galaxy

304 citations · 1.6k across the 12 of their papers we have counts for

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6 papers · 1 filter

astro-ph2006★ 199 cited

X-ray Supercavities in the Hydra A Cluster and the Outburst History of the Central Galaxy's Active Nucleus

M. W. Wise, B. R. McNamara, P. E. J. Nulsen +2

A 227 ksec Chandra Observatory X-ray image of the hot plasma in the Hydra A cluster has revealed an extensive cavity system. The system was created by a continuous outflow or a ser…

astro-ph2003★ 69 cited

Chandra High-Resolution X-Ray Spectrum of Supernova Remnant 1E0102.2-7219

K. A. Flanagan, C. R. Canizares, D. Dewey +5

Chandra High Energy Transmission Grating Spectrometer observations of the supernova remnant 1E0102.2-7219 in the Small Magellanic Cloud reveal a spectrum dominated by X-ray emissio…

astro-ph2001★ 227 cited

Discovery of Ghost Cavities in Abell 2597's X-ray Atmosphere

B. R. McNamara, M. W. Wise, P. E. J. Nulsen +10

A Chandra image of the central 100 kpc of the Abell 2597 cluster of galaxies shows bright, irregular, X-ray emission within the central dominant cluster galaxy (CDG), and two low s…

astro-ph2001

Ionization Structure and the Reverse Shock in E0102-72

K. A. Flanagan, C. R. Canizares, D. S. Davis +3

The young oxygen-rich supernova remnant E0102-72 in the Small Magellanic Cloud has been observed with the High Energy Transmission Grating Spectrometer of Chandra. The high resolut…

astro-ph2001

Spectral Line Imaging Observations of 1E0102.2-7219

D. S. Davis, K. A. Flanagan, J. C. Houck +5

E0102-72 is the second brightest X-ray source in the Small Magellanic Cloud and the brightest supernova remnant in the SMC. We observed this SNR for ~140 ksec with the High Energy…

astro-ph2000★ 176 cited

High Resolution X-Ray Spectra of Capella: Initial Results from the Chandra High Energy Transmission Grating Spectrometer

C. R. Canizares, D. P. Huenemoerder, D. S. Davis +10

High resolution spectra of the active binary Capella (G8 III + G1 III) covering the energy range 0.4-8.0 keV (1.5-30 Angstroms) show a large number of emission lines, demonstrating…