Search Results - "Kawata, D"
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Confirming chemical clocks: asteroseismic age dissection of the Milky Way disc(s)
Published in Monthly notices of the Royal Astronomical Society (01-04-2018)“…Abstract Investigations of the origin and evolution of the Milky Way disc have long relied on chemical and kinematic identifications of its components to…”
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Milky Way's thick and thin disk: Is there a distinct thick disk?
Published in Astronomische Nachrichten (01-09-2016)“…This article is based on our discussion session on Milky Way models at the 592 WE‐Heraeus Seminar, Reconstructing the Milky Way's History: Spectroscopic…”
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The history of the dark and luminous side of Milky Way-like progenitors
Published in Monthly notices of the Royal Astronomical Society (01-07-2017)“…Abstract Here we investigate the evolution of a Milky Way (MW)-like galaxy with the aim of predicting the properties of its progenitors all the way from z ∼ 20…”
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Thin disc, thick disc and halo in a simulated galaxy
Published in Monthly notices of the Royal Astronomical Society (11-10-2012)“…Abstract Within a cosmological hydrodynamical simulation, we form a disc galaxy with sub-components which can be assigned to a thin stellar disc, thick disc…”
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Galaxy formation with radiative and chemical feedback
Published in Monthly notices of the Royal Astronomical Society (21-05-2015)“…Here we introduce GAMESH, a novel pipeline that implements self-consistent radiative and chemical feedback in a computational model of galaxy formation. By…”
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Calibrating an updated smoothed particle hydrodynamics scheme within gcd
Published in Monthly notices of the Royal Astronomical Society (01-01-2013)“…We adapt a modern scheme of smoothed particle hydrodynamics (SPH) to our tree N-body/SPH galactic chemodynamics code gcd+. The applied scheme includes…”
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Mining the Galactic halo for very metal-poor stars
Published in Monthly notices of the Royal Astronomical Society. Letters (01-01-2010)“…We study the age and metallicity distribution function (MDF) of metal-poor stars in the Milky Way halo as a function of galactocentric radius by combining…”
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ramses‐ch: a new chemodynamical code for cosmological simulations
Published in Monthly notices of the Royal Astronomical Society. Letters (01-07-2012)“…ABSTRACT We present a new chemodynamical code –ramses‐ch– for use in simulating the self‐consistent evolution of chemical and hydrodynamical properties of…”
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PLATO as it is: A legacy mission for Galactic archaeology
Published in Astronomische Nachrichten (01-07-2017)“…Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high‐resolution chrono‐chemo‐kinematical…”
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GCD+: a new chemodynamical approach to modelling supernovae and chemical enrichment in elliptical galaxies
Published in Monthly notices of the Royal Astronomical Society (11-04-2003)“…We have developed a new galactic chemodynamical evolution code, called gcd+, for studies of galaxy formation and evolution.This code is based on our original…”
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Spiral arm kinematics for Milky Way stellar populations
Published in Monthly notices of the Royal Astronomical Society (21-09-2016)“…We present a new theoretical population synthesis model (the Galaxy model) to examine and deal with large amounts of data from surveys of the Milky Way and to…”
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Disc heating: comparing the Milky Way with cosmological simulations
Published in Monthly notices of the Royal Astronomical Society (01-08-2011)“…We present an analysis of a suite of simulations run with different particle- and grid-based cosmological hydrodynamical codes and compare them with…”
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Radial migration in numerical simulations of Milky-Way sized galaxies
Published in Astronomische Nachrichten (01-09-2016)“…We show that in rmN ‐body simulations of isolated spiral discs, spiral arms appear to transient, recurring features that co‐rotate with the stellar disc stars…”
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Chemodynamical analysis of bulge stars for simulated disc galaxies
Published in Monthly notices of the Royal Astronomical Society (21-01-2010)“…We analyse the kinematics and chemistry of the bulge stars of two simulated disc galaxies using our chemodynamical galaxy evolution code gcd+. First, we…”
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Multiwavelength cosmological simulations of elliptical galaxies
Published in Monthly notices of the Royal Astronomical Society (21-11-2003)“…We study the chemodynamical evolution of elliptical galaxies and their X-ray and optical properties using high-resolution cosmological simulations. Our tree…”
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Self-regulated active galactic nuclei heating in elliptical galaxies
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2005)“…We study the effect of active galactic nuclei (AGN) heating on the chemodynamical evolution of elliptical galaxies and their X-ray and optical properties using…”
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Are dry mergers dry, moist or wet?
Published in Monthly notices of the Royal Astronomical Society (11-12-2009)“…We present a spectral analysis of a sample of red-sequence galaxies identified by van Dokkum as dry merger remnants and ongoing dry mergers. Kinematics,…”
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Stellar dynamics around transient co-rotating spiral arms
Published in EPJ Web of conferences (01-01-2012)“…Spiral density wave theory attempts to describe the spiral pattern in spiral galaxies in terms of a long-lived wave structure with a constant pattern speed in…”
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High resolution science with high redshift galaxies
Published in Advances in space research (2008)“…We summarize the high-resolution science that has been done on high redshift galaxies with Adaptive Optics (AO) on the world’s largest ground-based facilities…”
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Cosmological simulations of the high-redshift radio universe
Published in Monthly notices of the Royal Astronomical Society (01-10-2004)“…ABSTRACT Using self‐consistent cosmological simulations of disc galaxy formation, we analyse the 1.4‐GHz radio flux from high‐redshift progenitors of…”
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