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20042026
most citedA Necessary Condition for Individual Time-Steps in SPH Simulations

194 citations · 2.5k across the 56 of their papers we have counts for

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Showing 2011Show all

6 papers · 1 filter

astro-ph.GA2011★ 21 cited

Origin of multiple nuclei in ultraluminous infrared galaxies

Hidenori Matsui, Takayuki R. Saitoh, Junichiro Makino +6

Ultraluminous infrared galaxies (ULIRGs) with multiple () nuclei are frequently observed. It has been suggested that these nuclei are produced by multiple major mergers of g…

astro-ph.CO2011★ 63 cited

Natures of a clump-origin bulge: a pseudobulge-like but old metal-rich bulge

Shigeki Inoue, Takayuki R. Saitoh

Bulges in spiral galaxies have been supposed to be classified into two types: classical bulges or pseudobulges. Classical bulges are thought to form by galactic merger with bursty…

astro-ph.CO2011★ 59 cited

Shallowed cusp slope of dark matter in disc galaxy formation through clump clusters

Shigeki Inoue, Takayuki R. Saitoh

Cusp-core problem is a controversial problem on galactic dark matter haloes. Cosmological N-body simulations has demonstrated that galactic dark matter haloes have a cuspy density…

astro-ph.GA2011★ 40 cited

Nuclear Star-Forming Ring of the Milky Way: Simulations

Sungsoo S. Kim, Takayuki R. Saitoh, Myoungwon Jeon +3

We present hydrodynamic simulations of gas clouds in the central kpc region of the Milky Way that is modeled with a three-dimensional bar potential. Our simulations consider realis…

astro-ph.GA2011★ 121 cited

Interplay between Stellar Spirals and the ISM in Galactic Disks

Keiichi Wada, Junichi Baba, Takayuki R. Saitoh

We propose a new dynamical picture of galactic stellar and gas spirals, based on hydrodynamic simulations in a `live' stellar disk. We focus especially on spiral structures excited…

astro-ph.CO2011★ 2 cited

Shock-induced star cluster formation in colliding galaxies

Takayuki R. Saitoh, Hiroshi Daisaka, Eiichiro Kokubo +5

We studied the formation process of star clusters using high-resolution N-body/smoothed particle hydrodynamcs simulations of colliding galaxies. The total number of particles is 1.…