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Astrometry and Celestial Mechanics

astrometry

celestial mechanics

eclipses

ephemerides

occultations

parallaxes

proper motions

time

Astronomical Databases

astronomical databases: miscellaneous

atlases

catalogs

surveys

virtual observatory tools

Astronomical Instrumentation, Methods and Techniques

atmospheric effects

instrumentation: miscellaneous

instrumentation: interferometers

instrumentation: photometers

instrumentation: spectrographs

instrumentation: detectors

instrumentation: polarimeters

instrumentation: adaptive optics

instrumentation: high angular resolution

light pollution

methods: analytical

methods: miscellaneous

methods: statistical

methods: observational

methods: numerical

methods: data analysis

methods: laboratory: molecular

methods: laboratory: solid state

site testing

space vehicles

space vehicles: instruments

techniques: interferometric

techniques: photometric

techniques: spectroscopic

techniques: polarimetric

techniques: miscellaneous

techniques: high angular resolution

techniques: image processing

techniques: imaging spectroscopy

techniques: radial velocities

telescopes

Cosmology

(cosmology:) inflation

(cosmology:) cosmic background radiation

(cosmology:) cosmological parameters

(cosmology:) dark energy

(cosmology:) dark matter

(cosmology:) dark ages, reionization, first stars

(cosmology:) diffuse radiation

(cosmology:) distance scale

(cosmology:) early universe

(cosmology:) large-scale structure of universe

cosmology: observations

cosmology: theory

cosmology: miscellaneous

Galaxies

(galaxies:) BL Lacertae objects: individual

(galaxies:) BL Lacertae objects: general

(galaxies:) intergalactic medium

(galaxies:) Local Group

(galaxies:) Magellanic Clouds

(galaxies:) quasars: general

(galaxies:) quasars: individual

(galaxies:) quasars: absorption lines

(galaxies:) quasars: emission lines

(galaxies:) quasars: supermassive black holes

galaxies: spiral

galaxies: general

galaxies: formation

galaxies: halos

galaxies: photometry

galaxies: nuclei

galaxies: statistics

galaxies: active

galaxies: structure

galaxies: Seyfert

galaxies: starburst

galaxies: abundances

galaxies: dwarf

galaxies: interactions

galaxies: high-redshift

galaxies: peculiar

galaxies: irregular

galaxies: jets

galaxies: ISM

galaxies: individual

galaxies: evolution

galaxies: bulges

galaxies: clusters: general

galaxies: clusters: individual

galaxies: clusters: intracluster medium

galaxies: distances and redshifts

galaxies: elliptical and lenticular, cD

galaxies: fundamental parameters

galaxies: groups: individual

galaxies: groups: general

galaxies: kinematics and dynamics

galaxies: luminosity function, mass function

galaxies: magnetic fields

galaxies: star formation

galaxies: star clusters: general

galaxies: stellar content

General

errata, addenda

history and philosophy of astronomy

miscellaneous

sociology of astronomy

Interstellar Medium (ISM), Nebulae

(ISM:) evolution

(ISM:) cosmic rays

(ISM:) dust, extinction

(ISM:) Herbig-Haro objects

(ISM:) HII regions

(ISM:) photon-dominated region (PDR)

(ISM:) planetary nebulae: general

(ISM:) planetary nebulae: individual

ISM: abundances

ISM: atoms

ISM: bubbles

ISM: molecules

ISM: clouds

ISM: structure

ISM: general

ISM: individual objects (except planetary nebulae)

ISM: jets and outflows

ISM: kinematics and dynamics

ISM: lines and bands

ISM: magnetic fields

ISM: supernova remnants

Physical Data and Processes

acceleration of particles

accretion, accretion disks

asteroseismology

astrobiology

astrochemistry

astroparticle physics

atomic processes

atomic data

black hole physics

chaos

conduction

convection

dense matter

diffusion

dynamo

elementary particles

equation of state

gravitation

gravitational waves

gravitational lensing: strong

gravitational lensing: weak

hydrodynamics

instabilities

line: formation

line: profiles

line: identification

magnetic reconnection

magnetic fields

magnetohydrodynamics (MHD)

masers

molecular processes

molecular data

neutrinos

nuclear reactions, nucleosynthesis, abundances

opacity

plasmas

polarization

radiation mechanisms: non-thermal

radiation mechanisms: general

radiation mechanisms: thermal

radiation: dynamics

radiative transfer

relativistic processes

scattering

shock waves

turbulence

waves

Planetary Systems

comets: individual

comets: general

Earth

interplanetary medium

Kuiper belt: general

meteorites, meteors, meteoroids

minor planets, asteroids: general

minor planets, asteroids: individual

Moon

planet-disk interactions

planets and satellites: composition

planets and satellites: detection

planets and satellites: individual

planets and satellites: formation

planets and satellites: rings

planets and satellites: general

planets and satellites: atmospheres

planets and satellites: surfaces

planets and satellites: oceans

planets and satellites: interiors

planets and satellites: aurorae

planets and satellites: dynamical evolution and stability

planets and satellites: fundamental parameters

planets and satellites: gaseous planets

planets and satellites: magnetic fields

planets and satellites: physical evolution

planets and satellites: terrestrial planets

planet-star interactions

protoplanetary disks

zodiacal dust

Resolved and Unresolved Sources as a Function of Wavelength

gamma rays: galaxies

gamma rays: stars

gamma rays: general

gamma rays: ISM

gamma rays: diffuse background

gamma rays: galaxies: clusters

infrared: stars

infrared: general

infrared: galaxies

infrared: ISM

infrared: diffuse background

infrared: planetary systems

radio continuum: general

radio continuum: galaxies

radio continuum: ISM

radio continuum: stars

radio lines: ISM

radio lines: stars

radio lines: galaxies

radio lines: general

submillimeter: ISM

submillimeter: galaxies

submillimeter: general

submillimeter: planetary systems

ultraviolet: stars

ultraviolet: planetary systems

X-rays: binaries

X-rays: individual

X-rays: ISM

X-rays: stars

X-rays: general

X-rays: galaxies

X-rays: bursts

X-rays: diffuse background

X-rays: galaxies: clusters

Stars

(stars:) supergiants

(stars:) subdwarfs

(stars:) starspots

(stars:) binaries (including multiple): close

(stars:) binaries: general

(stars:) binaries: eclipsing

(stars:) binaries: visual

(stars:) binaries: symbiotic

(stars:) binaries: spectroscopic

(stars:) blue stragglers

(stars:) brown dwarfs

(stars:) circumstellar matter

(stars:) gamma-ray burst: individual

(stars:) gamma-ray burst: general

(stars:) Hertzsprung-Russell and C-M diagrams

(stars:) novae, cataclysmic variables

(stars:) planetary systems

(stars:) pulsars: general

(stars:) pulsars: individual

(stars:) supernovae: general

(stars:) supernovae: individual

(stars:) white dwarfs

stars: interiors

stars: protostars

stars: mass-loss

stars: Wolf-Rayet

stars: carbon

stars: activity

stars: individual

stars: distances

stars: imaging

stars: jets

stars: flare

stars: coronae

stars: neutron

stars: low-mass

stars: statistics

stars: early-type

stars: general

stars: massive

stars: late-type

stars: horizontal-branch

stars: rotation

stars: evolution

stars: solar-type

stars: chromospheres

stars: atmospheres

stars: magnetars

stars: abundances

stars: formation

stars: AGB and post-AGB

stars: black holes

stars: chemically peculiar

stars: dwarf novae

stars: emission-line, Be

stars: fundamental parameters

stars: kinematics and dynamics

stars: luminosity function, mass function

stars: magnetic fields

stars: oscillations (including pulsations)

stars: peculiar (except chemically peculiar)

stars: Population II

stars: Population III

stars: pre-main sequence

stars: variables: Cepheids

stars: variables: general

stars: variables: delta Scuti

stars: variables: RR Lyrae

stars: variables: T Tauri, Herbig Ae/Be

stars: winds, outflows

The Sun

(Sun:) sunspots

(Sun:) solar wind

(Sun:) solar-terrestrial relations

Sun: corona

Sun: flares

Sun: evolution

Sun: granulation

Sun: activity

Sun: chromosphere

Sun: abundances

Sun: helioseismology

Sun: general

Sun: oscillations

Sun: atmosphere

Sun: infrared

Sun: photosphere

Sun: rotation

Sun: interior

Sun: coronal mass ejections (CMEs)

Sun: faculae, plages

Sun: filaments, prominences

Sun: fundamental parameters

Sun: magnetic fields

Sun: particle emission

Sun: radio radiation

Sun: transition region

Sun: UV radiation

Sun: X-rays, gamma rays

The Galaxy

(Galaxy:) globular clusters: individual

(Galaxy:) globular clusters: general

(Galaxy:) local interstellar matter

(Galaxy:) open clusters and associations: general

(Galaxy:) open clusters and associations: individual

(Galaxy:) solar neighborhood

Galaxy: disk

Galaxy: evolution

Galaxy: bulge

Galaxy: halo

Galaxy: abundances

Galaxy: nucleus

Galaxy: formation

Galaxy: general

Galaxy: structure

Galaxy: center

Galaxy: fundamental parameters

Galaxy: kinematics and dynamics

Galaxy: stellar content

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Journal Article

Particle–particle particle–tree code for planetary system formation with individual cut-off method: GPLUM

PDF

Yota Ishigaki and others

Publications of the Astronomical Society of Japan, Volume 73, Issue 3, June 2021, Pages 660–676, https://doi.org/10.1093/pasj/psab028

Published: 01 May 2021

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