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20032007
most citedA Half-Megasecond Chandra Observation of the Oxygen-Rich Supernova Remnant G292.0+1.8

73 citations · 184 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph200773 cited

A Half-Megasecond Chandra Observation of the Oxygen-Rich Supernova Remnant G292.0+1.8

Sangwook Park, John P. Hughes, Patrick O. Slane +3

We report on our initial analysis of a deep 510 ks observation of the Galactic oxygen-rich supernova remnant (SNR) G292.0+1.8 with the {\it Chandra X-ray Observatory}. Our new {\it…

astro-ph200738 cited

Observations of X-rays and Thermal Dust Emission from the Supernova Remnant Kes 75

T. D. Morton, P. Slane, K. J. Borkowski +4

We present Spitzer Space Telescope and Chandra X-ray Observatory observations of the composite Galactic supernova remnant Kes 75 (G29.7-0.3). We use the detected flux at 24 microns…

astro-ph2006

The X-ray Structure of the Pulsar Bow Shock G189.22+2.90 in the Supernova Remnant IC 443

B. M. Gaensler, S. Chatterjee, P. O. Slane +3

We present a deep observation with the Chandra X-ray Observatory of the neutron star bow shock G189.22+2.90 in the supernova remnant (SNR) IC 443. Our data confirm the cometary mor…

astro-ph2003

An X-ray study of the supernova remnant G18.95-1.1

Ilana M. Harrus, Patrick O. Slane, John P. Hughes +1

We present an analysis of data from both the Rontgen Satellite (ROSAT), and the Advanced Satellite for Cosmology and Astrophysics (ASCA) of the supernova remnant (SNR) G18.95-1.1.…

astro-ph2003

A High-Resolution Study of Nonthermal Radio and X-Ray Emission from SNR G347.3-0.5

J. S. Lazendic, P. O. Slane, B. M. Gaensler +3

G347.3-0.5 is one of three shell-type supernova remnants in the Galaxy whose X-ray spectrum is dominated by nonthermal emission. This puts G347.3-0.5 in the small, but growing clas…

astro-ph2003

X-ray Observations of the Compact Source in CTA 1

Patrick Slane, Erik R. Zimmerman, John P. Hughes +3

The point source RX J0007.0+7302, at the center of supernova remnant CTA 1, was studied using the X-Ray Multi-mirror Mission. The X-ray spectrum of the source is consistent with a…