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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2019
Abstract We study the dynamical properties of objects in hyperbolic orbits passing through the inner Solar system in the context of two different potential... 
Journal Article
Proceedings of the International Astronomical Union, ISSN 1743-9213, 08/2018, Volume 14, Issue S345, pp. 141 - 147
AbstractIn the standard formation scenario of planetary systems, planets form from a protoplanetary disk that consists of gas and dust. The scenario can be... 
Terrestrial planets | Dust | Protoplanets | Planet formation | Terrestrial environments | Coagulation | Protoplanetary disk | Embryos | Pluto | Planetary systems
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2018, Volume 481, Issue 1, pp. 185 - 193
The origin of galactic spiral arms is one of the fundamental problems in astrophysics. Based on the local analysis, Toomre (1981) proposed the swing... 
Galaxies: spiral | Methods: numerical | DISK GALAXIES | ORIGIN | PARTICLES | MODELS | X86 ARCHITECTURE | ASTRONOMY & ASTROPHYSICS | SIMD INSTRUCTION SET | STARS | methods: numerical | galaxies: spiral | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2017, Volume 842, Issue 1, p. 61
We consider the dynamics of porous icy dust aggregates in a turbulent gas disk and investigate the stability of the disk. We evaluate the random velocity of... 
planets and satellites: formation | protoplanetary disks | GALACTIC SPIRAL ARMS | HEAD-ON COLLISIONS | SHEAR INSTABILITIES | ASTRONOMY & ASTROPHYSICS | SOLAR NEBULA | SWING AMPLIFICATION | PLANETESIMAL FORMATION | MAGNETOROTATIONAL INSTABILITY | NUMERICAL-SIMULATION | N-BODY SIMULATION | Physics - Earth and Planetary Astrophysics
Journal Article
Journal Article
Astrophysical Journal, ISSN 0004-637X, 04/2016, Volume 821, Issue 1, pp. 35 - 35
Based on the swing amplification model of Julian & Toomre, we investigate the formation and structure of stellar spirals in disk galaxies. We calculate the... 
methods: numerical | galaxies: spiral | galaxies: kinematics and dynamics | DENSITY WAVES | SHEARING SHEET | STABILITY | PITCH-ANGLE | EVOLUTION | MODELS | ASTRONOMY & ASTROPHYSICS | DYNAMICS | SIMULATIONS | DISK | Amplification | Wavelengths | Swing | Disk galaxies | Pitch angle | Mathematical models | Dynamical systems | Shear rate | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2016, Volume 823, Issue 2, pp. 121 - 121
We revisit the swing amplification model of galactic spiral arms proposed by Toomre. We describe the derivation of the perturbation equation in detail and... 
methods: analytical | galaxies: spiral | galaxies: kinematics and dynamics | DENSITY WAVES | DISK GALAXIES | ASTRONOMY & ASTROPHYSICS | MODAL APPROACH | DYNAMICS | PITCH-ANGLE | SIMULATIONS | MORPHOLOGY | Amplification | Galactic structure | Spirals | Synchronism | Swing | Pitch angle | Mathematical models | Synchronization | Physics - Astrophysics of Galaxies
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 405, Issue 2, pp. 1227 - 1243
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 12/2002, Volume 581, Issue 1 I, pp. 666 - 680
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 03/2017, Volume 837, Issue 1, pp. L13 - L13
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 12/2019, Volume 886, Issue 2, p. 107
As a natural consequence of the elementary processes of dust growth, we discovered that a new class of planets can be formed around supermassive black holes... 
Planetary system formation | Active galactic nuclei | DUST | EVOLUTION | Supermassive black holes | Interstellar dust | DISKS | ASTRONOMY & ASTROPHYSICS | Exoplanet formation | COAGULATION | TURBULENCE | EMISSION
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 07/2016, Volume 825, Issue 2, pp. L28 - L28
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2018, Volume 855, Issue 1, p. 57
Planetesimal formation is one of the most important unsolved problems in planet formation theory. In particular, rocky planetesimal formation is difficult... 
methods: analytical | protoplanetary disks | instabilities | planets and satellites: formation | HEAD-ON COLLISIONS | COMPRESSION | DISRUPTION | EVOLUTION | DRAG | ASTRONOMY & ASTROPHYSICS | GROWTH | SOLAR NEBULA | PLANETESIMAL FORMATION | NUMERICAL-SIMULATION | N-BODY SIMULATION | Physics - Earth and Planetary Astrophysics
Journal Article
The Astrophysical Journal Letters, ISSN 2041-8205, 05/2010, Volume 714, Issue 1, pp. L21 - L25
The final stage of terrestrial planet formation is known as the giant impact stage where protoplanets collide with one another to form planets. So far this... 
Planets and satellites: formation | Methods: numerical | PLANETESIMALS | HERMITE INTEGRATOR | ASTRONOMY & ASTROPHYSICS | GROWTH | methods: numerical | IMPACTS | planets and satellites: formation | N-BODY SIMULATION | Physics - Earth and Planetary Astrophysics
Journal Article
Astrophysical Journal Letters, ISSN 2041-8205, 05/2010, Volume 714, Issue 1
The final stage of terrestrial planet formation is known as the giant impact stage where protoplanets collide with one another to form planets. So far this... 
PLANETS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | IMPACT PARAMETER | MASS | GENERAL AND MISCELLANEOUS//MATHEMATICS, COMPUTING, AND INFORMATION SCIENCE | PROTOPLANETS | SATELLITES | SIMULATION | ANGULAR VELOCITY
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 8/2012, Volume 424, Issue 2, pp. 1419 - 1431
Journal Article
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