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Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2018, Volume 473, Issue 2, pp. 1718 - 1718
Journal Article
2010, ISBN 0521517729, xviii, 377
Planet formation studies uniquely benefit from three disciplines: astronomical observations of extrasolar planet-forming disks, analysis of material from the... 
Protoplanetary disks
Book
Chemical Reviews, ISSN 0009-2665, 12/2013, Volume 113, Issue 12, pp. 9016 - 9042
Henning and Semenov examine the role of chemistry with regard to protoplanetary disks. 
Protoplanets | Planet formation
Journal Article
by Wang, Y and Zho, JL and Liu, FY and Sun, W and Liu, HG and Yang, M
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 11/2019, Volume 490, Issue 1, pp. 359 - 370
A type of compactly spaced and comparably sized multi-exoplanet system similar to TRAPPIST-1 has been discovered recently. The stability of these systems is an... 
Planetary System | PROTOPLANET | planets and satellites: dynamical evolution and stability | RESONANCE OVERLAP | BEHAVIOR | ASTRONOMY & ASTROPHYSICS
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 11/2004, Volume 616, Issue 1 I, pp. 567 - 572
The apparent dependence of detection frequency of extrasolar planets on the metallicity of their host stars is investigated with Monte Carlo simulations using... 
Planetary systems: formation | Solar system: formation | Stars: statistics | DENSITY WAVES | PLANETESIMALS | EXTRASOLAR PLANETS | EVOLUTION | ASTRONOMY & ASTROPHYSICS | SOLAR NEBULA | ACCRETION | ORBITAL MIGRATION | NUMERICAL SIMULATIONS | PROTOPLANET | DISK
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 10/2019, Volume 489, Issue 2, pp. 2159 - 2176
We investigate planetesimal accretion via a direct N-body simulation of an annulus at 1 au orbiting a 1 M-circle dot star. The planetesimal ring, which... 
MIGRATION | VELOCITY | SWARM | methods: numerical | PLANETESIMALS | EVOLUTION | ASTRONOMY & ASTROPHYSICS | ACCRETION | OLIGARCHIC GROWTH | PROTOPLANET | planets and satellites: formation | NUMERICAL-SIMULATION | DISK | Physics - Earth and Planetary Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 405, Issue 3, pp. 1473 - 1490
Journal Article
Icarus, ISSN 0019-1035, 2009, Volume 201, Issue 1, pp. 381 - 394
An investigation of the stability of systems of 1 (Earth-mass) bodies orbiting a Sun-like star has been conducted for virtual times reaching 10 billion years.... 
Extrasolar planets | Planetary dynamics | Celestial mechanics | PROTOPLANET SYSTEM | INSTABILITY | ASTRONOMY & ASTROPHYSICS | DYNAMICS | Mechanical engineering | Planets
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 465, Issue 1, pp. 1089 - 1089
The dynamics of dust and gas can be quite different from each other when the dust is poorly coupled to the gas. In protoplanetary discs, it is well known that... 
Collapse | Dust | Star formation | Protoplanets | Grains | Planet formation | Dynamics | Protostars
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 02/2017, Volume 465, Issue 2, pp. 1910 - 1910
Ices, including water ice, prefer to recondense on to preexisting nuclei rather than spontaneously forming grains from a cloud of vapour. Interestingly,... 
Protoplanets | Grains | Planet formation | Formations | Outbursts | Vapour | Solar system | Nuclei
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2016, Volume 463, Issue 3, pp. 2480 - 2480
We investigate the conditions required for planet formation via gravitational instability (GI) and protoplanetary disc (PPD) fragmentation around M-dwarfs.... 
Protoplanets | Initial conditions | Planet formation | Disks | Clumps | Mathematical models | Fragmentation
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2016, Volume 463, Issue 4, pp. 4167 - 4167
We consider the mechanism of photophoretic transport in protoplanetary discs that are optically thick to radiation. Here, photophoresis is not caused by the... 
Bouncing | Dust | Protoplanets | Aggregates | Planet formation | Fluctuation | Chondrule | Mass transfer
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2016, Volume 462, Issue 4, pp. 4549 - 4549
Recently it has been proposed that the zombie vortex instability (ZVI) could precipitate hydrodynamical activity and angular momentum transport in unmagnetized... 
Operators | Protoplanets | Planet formation | Vortices | Fluid flow | Disks | Instability | Diffusion
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2016, Volume 460, Issue 2, pp. 2103 - 2103
New calculations for rotational excitation of cyanoacetylene by collisions with hydrogen molecules are performed to include the lowest 38 rotational levels of... 
Coupling (molecular) | Cyanoacetylene | Spectroscopy | Protoplanets | Mathematical analysis | Collisions | Excitation | Rotational
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 08/2016, Volume 460, Issue 3, pp. 2482 - 2482
We explore the possibility of planet formation in the carbon-rich protoplanetary discs of carbon-enhanced metal-poor (CEMP) stars, possible relics of the early... 
Planets | Transits | Protoplanets | Planet formation | Stars | Abundance | Universe | Carbon
Journal Article
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