Search Results - "RICH, R. R"
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Exact Traveling Wave Solutions in Viscoelastic Channel Flow
Published in Physical review letters (06-10-2020)“…Elasto-inertial turbulence (EIT) is a new, two-dimensional chaotic flow state observed in polymer solutions with possible connections to inertialess elastic…”
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Mitochondrial cytochrome c oxidase: catalysis, coupling and controversies
Published in Biochemical Society transactions (15-06-2017)“…Mitochondrial cytochrome oxidase is a member of a diverse superfamily of haem-copper oxidases. Its mechanism of oxygen reduction is reviewed in terms of the…”
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Stellar halos in Illustris: probing the histories of Milky Way-mass galaxies
Published in Monthly notices of the Royal Astronomical Society (21-09-2018)Get full text
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Pristine dwarf galaxy survey – I. A detailed photometric and spectroscopic study of the very metal-poor Draco II satellite
Published in Monthly notices of the Royal Astronomical Society (21-10-2018)“…We present a detailed study of the faint Milky Way satellite Draco II (Dra II) from deep CFHT/MegaCam broad-band g and i photometry and narrow-band…”
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A CHEMICAL CONFIRMATION OF THE FAINT BOÖTES II DWARF SPHEROIDAL GALAXY
Published in The Astrophysical journal (10-10-2014)“…We present a chemical abundance study of the brightest confirmed member star of the ultra-faint dwarf galaxy Bootes II from Keck/HIRES high-resolution…”
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Recurrent flow patterns as a basis for two-dimensional turbulence: Predicting statistics from structures
Published in Proceedings of the National Academy of Sciences - PNAS (04-06-2024)“…A dynamical systems approach to turbulence envisions the flow as a trajectory through a high-dimensional state space [Hopf, , 303 (1948)]. The chaotic dynamics…”
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A new model for the Milky Way bar
Published in Monthly notices of the Royal Astronomical Society (01-12-2012)“…We use Schwarzschild's orbit-superposition technique to construct self-consistent models of the Galactic bar. Using χ2 minimization, we find that the…”
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Quantified diffuse light in compact groups of galaxies
Published in Monthly notices of the Royal Astronomical Society (01-06-2021)“…ABSTRACT The vast majority of stars in galaxy groups are contained within their constituent galaxies. Some small fraction of stars is expected, however, to…”
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The haloes and environments of nearby galaxies (HERON) – I. Imaging, sample characteristics, and envelope diameters
Published in Monthly notices of the Royal Astronomical Society (01-12-2019)“…We use a dedicated 0.7-m telescope to image the haloes of 119 galaxies in the Local Volume to μr ∼ 28–30 mag arcsec−2. The sample is primarily from the Two…”
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Wall shear stress and pressure patterns in aortic stenosis patients with and without aortic dilation captured by high-performance image-based computational fluid dynamics
Published in PLoS computational biology (18-10-2023)“…Spatial patterns of elevated wall shear stress and pressure due to blood flow past aortic stenosis (AS) are studied using GPU-accelerated patient-specific…”
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The Ages of Galactic Bulge Stars with Realistic Uncertainties
Published in The Astrophysical journal (01-03-2023)“…Using modern isochrones with customized physics and carefully considered statistical techniques, we recompute the age distribution for a sample of 91…”
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THE AGE OF THE YOUNG BULGE-LIKE POPULATION IN THE STELLAR SYSTEM TERZAN 5: LINKING THE GALACTIC BULGE TO THE HIGH-Z UNIVERSE
Published in The Astrophysical journal (10-09-2016)“…The Galactic bulge is dominated by an old, metal-rich stellar population. The possible presence and the amount of a young (a few gigayears old) minor component…”
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The Pristine Dwarf-Galaxy survey – II. In-depth observational study of the faint Milky Way satellite Sagittarius II
Published in Monthly notices of the Royal Astronomical Society (01-01-2020)“…We present an extensive study of the Sagittarius II (Sgr II) stellar system using MegaCam g and i photometry, narrow-band, metallicity-sensitive calcium H&K…”
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Heat transport in Rayleigh-Bénard convection with linear marginality
Published in Philosophical transactions of the Royal Society of London. Series A: Mathematical, physical, and engineering sciences (13-06-2022)“…Recent direct numerical simulations (DNS) and computations of exact steady solutions suggest that the heat transport in Rayleigh-Bénard convection (RBC)…”
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THE PAndAS VIEW OF THE ANDROMEDA SATELLITE SYSTEM. II. DETAILED PROPERTIES OF 23 M31 DWARF SPHEROIDAL GALAXIES
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT We present a comprehensive analysis of the structural properties and luminosities of the 23 dwarf spheroidal galaxies that fall within the footprint…”
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The cluster Terzan 5 as a remnant of a primordial building block of the Galactic bulge
Published in Nature (London) (26-11-2009)“…Globular star clusters are compact and massive stellar systems old enough to have witnessed the entire history of our Galaxy, the Milky Way. Although recent…”
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The Hubble Space Telescope Survey of M31 Satellite Galaxies. I. RR Lyrae–based Distances and Refined 3D Geometric Structure
Published in The Astrophysical journal (01-10-2022)“…We measure homogeneous distances to M31 and 38 associated stellar systems (−16.8 ≤ M V ≤ −6.0), using time-series observations of RR Lyrae stars taken as part…”
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A New Generation of Cool White Dwarf Atmosphere Models. III. WD J2356-209: Accretion of a Planetesimal with an Unusual Composition
Published in The Astrophysical journal (20-02-2019)“…WD J2356−209 is a cool metal-polluted white dwarf whose visible spectrum is dominated by a strong and broad sodium feature. Although it was discovered nearly…”
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Detailed Abundances in the Galactic Center: Evidence of a Metal-rich Alpha-enhanced Stellar Population
Published in The Astrophysical journal (01-05-2020)“…We present a detailed study of the composition of 20 M giants in the Galactic center with 15 of them confirmed to be in the nuclear star cluster. As a control…”
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Formation of the Andromeda giant stream: asymmetric structure and disc progenitor
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…We focus on the evidence of a past minor merger discovered in the halo of the Andromeda galaxy (M31). Previous N-body studies have enjoyed moderate success in…”
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