Search Results - "FUJII, M. S"

THE FORMATION AND DYNAMICAL EVOLUTION OF YOUNG STAR CLUSTERS by Fujii, M. S., Zwart, S. Portegies

“…ABSTRACT Recent observations have revealed a variety of young star clusters, including embedded systems, young massive clusters, and associations. We study the…”
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Spin misalignment of black hole binaries from young star clusters: implications for the origin of gravitational waves events by Trani, A A, Tanikawa, A, Fujii, M S, Leigh, N W C, Kumamoto, J

“…ABSTRACT Recent studies indicate that the progenitors of merging black hole (BH) binaries from young star clusters can undergo a common envelope phase just…”
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Trimodal structure of Hercules stream explained by originating from bar resonances by Asano, Tetsuro, Fujii, M S, Baba, J, Bédorf, J, Sellentin, E, Portegies Zwart, S

“…ABSTRACT Gaia Data Release 2 revealed detailed structures of nearby stars in phase space. These include the Hercules stream, whose origin is still debated…”
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THE FORMATION OF YOUNG DENSE STAR CLUSTERS THROUGH MERGERS by FUJII, M. S, SAITOH, T. R, PORTEGIES ZWART, S. F

“…Young star clusters such as NGC 3603 and Westerlund 1 and 2 in the Milky Way and R136 in the Large Magellanic Cloud are dynamically more evolved than expected…”
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The Dynamics of Spiral Arms in Pure Stellar Disks by Fujii, M. S, Baba, J, Saitoh, T. R, Makino, J, Kokubo, E, Wada, K

“…It has been believed that spiral arms in pure stellar disks, especially the ones spontaneously formed, decay in several galactic rotations due to the increase…”
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The growth of massive stars via stellar collisions in ensemble star clusters by Fujii, M. S., Portegies Zwart, S.

“…Recent simulations and observations suggest that star clusters form via the assembling of smaller subclusters. Because of their short relaxation time,…”
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Kinematics of subclusters in star cluster complexes: imprint of their parental molecular clouds by Fujii, M S

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Modelling the Milky Way as a dry Galaxy by Fujii, M S, Bédorf, J, Baba, J, Portegies Zwart, S

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The dynamics of stellar discs in live dark-matter haloes by Fujii, M S, Bédorf, J, Baba, J, Portegies Zwart, S

“…Abstract Recent developments in computer hardware and software enable researchers to simulate the self-gravitating evolution of galaxies at a resolution…”
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The initial mass function of star clusters that form in turbulent molecular clouds by Fujii, M. S., Portegies Zwart, S.

“…We simulate the formation and evolution of young star clusters using the combination of smoothed particle hydrodynamics (SPH) simulations and direct N-body…”
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The moment of core collapse in star clusters with a mass function by Fujii, M. S., Portegies Zwart, S.

“…Star clusters with multimass components dynamically evolve faster than those modelled with equal-mass components. Using a series of direct N-body simulations,…”
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Destruction of star clusters due to the radial migration in spiral galaxies by Fujii, M. S., Baba, J.

“…ABSTRACT Most stars in galactic discs are believed to be born as a member of star clusters or associations. Star clusters formed in discs are disrupted due to…”
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Kinematics of Subclusters in Star Cluster Complexes: Imprint of their Parental Molecular Clouds by Fujii, M. S

“…Star cluster complexes such as the Carina Nebula can have formed in turbulent giant molecular clouds. We perform a series of $N$-body simulations starting from…”
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SIRIUS project II: a new tree-direct hybrid code for smoothed particle hydrodynamics/N-body simulations of star clusters by Fujii, M. S, Saitoh, T. R, Wang, L, Hirai, Y

“…Star clusters form via clustering star formation inside molecular clouds. In order to understand the dynamical evolution of star clusters in their early phase,…”
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Survival Rates of Planets in Open Clusters: the Pleiades, Hyades, and Praesepe clusters by Fujii, M. S, Hori, Y

“…A&A 624, A110 (2019) In clustered environments, stellar encounters can liberate planets from their host stars via close encounters. Although the detection…”
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Modelling the Milky Way as a dry Galaxy by Fujii, M. S., Bédorf, J., Baba, J., Portegies Zwart, S.

“…We construct a model for the Milky Way (MW) Galaxy composed of a stellar disc and bulge embedded in a dark-matter halo. All components are modelled as N-body…”
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The initial mass function of star clusters that form in turbulent molecular clouds by Fujii, M. S, Zwart, S. Portegies

“…We simulate the formation and evolution of young star clusters using the combination of SPH simulations and direct N-body simulations. We start by performing…”
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Destruction of star clusters due to the radial migration in spiral galaxies by Fujii, M. S, Baba, J

“…Most stars in galactic disks are believed to be born as a member of star clusters or associations. Star clusters formed in disks are disrupted due to the tidal…”
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The moment of core collapse in star clusters with a mass function by Fujii, M. S, Zwart, S. Portegies

“…Star clusters with multi-mass components dynamically evolve faster than those modeled with equal-mass components. Using a series of direct $N$-body…”
Get full text

The growth of massive stars via stellar collisions in ensemble star clusters by Fujii, M. S, Zwart, S. Portegies

“…Recent simulations and observations suggest that star clusters form via the assembling of smaller sub-clusters. Because of their short relaxation time,…”
Get full text