J. Regis McNamara
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View article: Cold Gas and Star Formation in the Phoenix Cluster with JWST
Cold Gas and Star Formation in the Phoenix Cluster with JWST Open
We present integral field unit observations of the Phoenix Cluster with the JWST Mid-infrared Instrument's Medium Resolution Spectrometer (MIRI/MRS). We focus this study on the molecular gas, dust, and star formation in the brightest clust…
View article: Cocoon shock, X-ray cavities, and extended inverse Compton emission in Hercules A: Clues from <i>Chandra</i> observations
Cocoon shock, X-ray cavities, and extended inverse Compton emission in Hercules A: Clues from <i>Chandra</i> observations Open
Aims. We present a detailed analysis of jet activity in the radio galaxy 3C 348 at the center of the galaxy cluster Hercules A. We aim to investigate the jet-driven shock fronts, the radio-faint X-ray cavities, the eastern jet, and the pre…
View article: Variation in treatment of intrahepatic cholangiocarcinoma: a nationwide multicentre study
Variation in treatment of intrahepatic cholangiocarcinoma: a nationwide multicentre study Open
Journal Article Variation in treatment of intrahepatic cholangiocarcinoma: a nationwide multicentre study Get access Jane McClements, Jane McClements Department of HPB Surgery, Nottingham University Hospitals NHS Trust, Nottingham, UK Sear…
View article: CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA
CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA Open
We present multiband photometry of 185 type-Ia supernovae (SNe Ia), with over 11,500 observations. These were acquired between 2001 and 2008 at the F. L. Whipple Observatory of the Harvard-Smithsonian Center for Astrophysics (CfA). This sa…
View article: Thermal Instability in Low Entropy Gas Lifted behind Buoyantly-Rising X-ray Bubbles
Thermal Instability in Low Entropy Gas Lifted behind Buoyantly-Rising X-ray Bubbles Open
Precipitation models indicate that cooling instabilities form when the ratio of cooling time to free-fall in hot atmospheres surrounding massive galaxies falls below ~10, i.e., t_c/t_ff < 10. We show that this criterion is rarely met in ce…