activity
19992003
most citedHigh Resolution X-Ray Spectra of Capella: Initial Results from the Chandra High Energy Transmission Grating Spectrometer

176 citations · 389 across the 8 of their papers we have counts for

collaborators

7 papers

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★ 28 cited

A Chandra HETG Observation of the Quasar H 1821+643 and Its Surrounding Cluster

T. Fang, D. S. Davis, J. C. Lee +3

We present the high-resolution X-ray spectrum of the low-redshift quasar H 1821+643 and its surrounding hot cluster observed with the Chandra High Energy Transmission Grating Spect…

astro-ph2001★ 8 cited

ASCA observations of massive medium-distant clusters of galaxies. II

H. Matsumoto, M. Pierre, T. G. Tsuru +1

We have selected seven medium-distant clusters of galaxies (z ~ 0.1 - 0.3) for multi-wavelength observations with the goal of investigating their dynamical state. Following Paper I…

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…

astro-ph1999★ 39 cited

Gas, Iron and Gravitational Mass in Galaxy Clusters: The General Lack of Cluster Evolution at z < 1.0

Hironori Matsumoto, Takeshi Go Tsuru, Yasushi Fukazawa +2

We have analyzed the ASCA data of 29 nearby clusters of galaxies systematically, and obtained temperatures, iron abundances, and X-ray luminosities of their intracluster medium (IC…