Search Results - "Johnstone, M R"
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Avibactam and class C β-lactamases: mechanism of inhibition, conservation of the binding pocket, and implications for resistance
Published in Antimicrobial agents and chemotherapy (01-10-2014)“…Avibactam is a novel non-β-lactam β-lactamase inhibitor that inhibits a wide range of β-lactamases. These include class A, class C, and some class D enzymes,…”
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A very deep Chandra observation of the Perseus cluster: shocks, ripples and conduction
Published in Monthly notices of the Royal Astronomical Society (01-02-2006)“…ABSTRACT We present the first results from a very deep Chandra X‐ray observation of the core of the Perseus cluster of galaxies. A pressure map reveals a clear…”
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A wide Chandra view of the core of the Perseus cluster
Published in Monthly notices of the Royal Astronomical Society (21-12-2011)“…We present new Chandra images of the X-ray emission from the core of the Perseus cluster of galaxies. The total observation time is now 1.4 Ms. New depressions…”
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Magnetic support of the optical emission line filaments in NGC 1275
Published in Nature (21-08-2008)“…The giant elliptical galaxy NGC 1275, at the centre of the Perseus cluster, is surrounded by a well-known giant nebulosity of emission-line filaments 1 , 2 ,…”
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Collisional heating as the origin of filament emission in galaxy clusters
Published in Monthly notices of the Royal Astronomical Society (01-02-2009)“…It has long been known that photoionization, whether by starlight or other sources, has difficulty in accounting for the observed spectra of the optical…”
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A deep Chandra observation of the Perseus cluster: shocks and ripples
Published in Monthly notices of the Royal Astronomical Society (21-09-2003)“…We present preliminary results from a deep observation lasting almost 200 ks of the centre of the Perseus cluster of galaxies around NGC 1275. The X-ray…”
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On the origin and excitation of the extended nebula surrounding NGC 1275
Published in Monthly notices of the Royal Astronomical Society (01-04-2006)“…We use line-of-sight velocity information on the filamentary emission-line nebula of NGC 1275 to infer a dynamical model of the nebula's flow through the…”
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Cool X-ray emitting gas in the core of the Centaurus cluster of galaxies
Published in Monthly notices of the Royal Astronomical Society (01-04-2008)“…We use a deep XMM–Newton Reflection Grating Spectrometer observation to examine the X-ray emission from the core of the Centaurus cluster of galaxies. We…”
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The nature of the molecular gas system in the core of NGC 1275
Published in Monthly notices of the Royal Astronomical Society (11-05-2005)“…We present near-infrared integral field spectroscopy of the central kiloparsec of NGC 1275 at the heart of the Perseus cluster of galaxies, obtained with the…”
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The X-ray luminous cluster underlying the bright radio-quiet quasar H1821+643
Published in Monthly notices of the Royal Astronomical Society (01-03-2010)“…We present a Chandra observation of the only low redshift, z= 0.299, galaxy cluster to contain a highly luminous radio-quiet quasar, H1821+643. By simulating…”
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A multiwavelength view of cooling versus AGN heating in the X-ray luminous cool-core of Abell 3581
Published in Monthly notices of the Royal Astronomical Society (21-10-2013)“…We report the results of a multiwavelength study of the nearby galaxy group, Abell 3581 (z = 0.0218). This system hosts the most luminous cool core of any…”
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Chandra imaging of the complex X-ray core of the Perseus cluster
Published in Monthly notices of the Royal Astronomical Society (11-11-2000)“…We report subarcsec-resolution X-ray imaging of the core of the Perseus cluster around the galaxy NGC 1275 with the Chandra X-ray Observatory. The…”
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Dynamical analysis of galaxy cluster merger Abell 2146
Published in Monthly notices of the Royal Astronomical Society (01-11-2015)“…We present a dynamical analysis of the merging galaxy cluster system Abell 2146 using spectroscopy obtained with the Gemini Multi-Object Spectrograph on the…”
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Discovery of atomic and molecular mid-infrared emission lines in off-nuclear regions of NGC 1275 and NGC 4696 with the Spitzer Space Telescope
Published in Monthly notices of the Royal Astronomical Society (11-12-2007)“…We present Spitzer high-resolution spectra of off-nuclear regions in the central cluster galaxies NGC 1275 and NGC 4696 in the Perseus and Centaurus clusters,…”
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The origin of molecular hydrogen emission in cooling-flow filaments
Published in Monthly notices of the Royal Astronomical Society. Letters (01-05-2008)“…The optical filaments found in many cooling flows in galaxy clusters consist of low-density (∼103 cm−3) cool (∼103 K) gas surrounded by significant amounts of…”
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Star formation in the outer filaments of NGC 1275
Published in Monthly notices of the Royal Astronomical Society (11-06-2010)“…We present photometry of the outer star clusters in NGC 1275, the brightest galaxy in the Perseus cluster. The observations were taken using the Hubble Space…”
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The prevalence of cooling cores in clusters of galaxies at z ≈ 0.15–0.4
Published in Monthly notices of the Royal Astronomical Society (01-06-2005)“…We present a Chandra study of 38 X-ray-luminous clusters of galaxies in the ROSAT Brightest Cluster Sample (BCS) that lie at moderate redshifts (z ≈ 0.15–0.4)…”
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Detections of molecular hydrogen in the outer filaments of NGC 1275
Published in Monthly notices of the Royal Astronomical Society (11-04-2005)“…We present clear spectroscopic detections of molecular hydrogen in the outer filaments of the Hα nebula surrounding the central galaxy of the Perseus cluster,…”
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A deep spectroscopic study of the filamentary nebulosity in NGC4696, the brightest cluster galaxy in the Centaurus cluster
Published in Monthly notices of the Royal Astronomical Society (01-11-2011)“…ABSTRACT We present results of deep integral-field spectroscopy observations using high-resolution optical (4150-7200Å) VLT VIsible MultiObject Spectrograph…”
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A ROSAT study of the cores of clusters of galaxies — I. Cooling flows in an X-ray flux-limited sample
Published in Monthly notices of the Royal Astronomical Society (01-08-1998)“…This is the first part of a study of the detailed X-ray properties of the cores of nearby clusters. We have used the flux-limited sample of 55 clusters listed…”
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