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Astrophysical Journal, ISSN 0004-637X, 11/2013, Volume 778, Issue 1, pp. 1 - 11
We infer the period (P) and size (R sub(p)) distribution of Kepler transiting planet candidates with R sub(p) [> or =, slanted] 1 R sub([+ in cirlced]) and P <... 
techniques: photometric | stars: statistics | planetary systems | Planets | Planet detection | Extrasolar planets | Mathematical analysis | Stars | Flats | Criteria | Distribution functions | DISTRIBUTION | STATISTICS | JUPITER PLANET | NOISE | RISE | DISTRIBUTION FUNCTIONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | IMPACT PARAMETER | MASS | STARS | DETECTION | EFFICIENCY | VISIBLE RADIATION | INDIUM FLUORIDES | NEPTUNE PLANET
Journal Article
Nature, ISSN 0028-0836, 11/2015, Volume 527, Issue 7578, pp. 310 - 311
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 11/2019
Abstract Recent observations have revealed a gallery of substructures in the dust component of nearby protoplanetary discs, including rings, gaps, spiral arms,... 
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 458, Issue 4, pp. 3918 - 3918
Motivated by lopsided structures observed in some massive transition discs, we have carried out 2D numerical simulations to study vortex structure in massive... 
Dust | Computer simulation | Vortices | Stars | Fluid flow | Disks | Mathematical models | Scale height
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 458, Issue 4, pp. 3927 - 3927
We investigate the dynamics of large dust grains in massive lopsided transition discs via 2D hydrodynamical simulations including both gas and dust. Our... 
Orbitals | Trapping | Dust | Simulation | Grains | Vortices | Fluid flow | Disks
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2016, Volume 458, Issue 4, pp. 3918 - 3926
Motivated by lopsided structures observed in some massive transition discs, we have carried out 2D numerical simulations to study vortex structure in massive... 
Hydrodynamics | Stars: Protostars | Instabilities | Protoplanetary discs | Physics | Astrophysics
Journal Article
中文自修, ISSN 1000-7245, 2015, Issue 24, pp. 36 - 36
来吧,小牛,去找妈妈,来吧,小羊,我选了你,来吧,小猫,一只又只,有雪白的爪乇来吧,小鹅,一身黄毛,跟着伙伴,跑上前来。 
诗歌 | 语文学习 | 阅读知识 | 课外阅读 | 小学生
Journal Article
by Zhu, ZH
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 03/2019, Volume 483, Issue 3, pp. 4221 - 4241
Journal Article
by Zhu, ZH
NATURE, ISSN 0028-0836, 11/2015, Volume 527, Issue 7578, pp. 310 - 311
Finding young planets in their birthplaces is extremely challenging, because actively forming planetary systems are far away and obscured by dust. On page 342... 
MAGNETOSPHERIC ACCRETION | CANDIDATE | T-TAURI STARS | DISK | MULTIDISCIPLINARY SCIENCES | Orbits | Planets | Astronomical research | Solar systems | Planetology
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 11/2013, Volume 778, Issue 1, p. 53
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2018, Volume 859, Issue 2, p. 118
Protoplanetary disk simulations show that a single planet can excite more than one spiral arm, possibly explaining the recent observations of multiple spiral... 
waves | hydrodynamics | planet-disk interactions | DENSITY WAVES | EXCITATION | EVOLUTION | ASTRONOMY & ASTROPHYSICS | LINDBLAD | THIN ACCRETION DISKS | ROSSBY-WAVE INSTABILITY | SHOCKS | Physics - Earth and Planetary Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 06/2018, Volume 859, Issue 2, p. 119
We examine whether various characteristics of planet-driven spiral arms can be used to constrain the masses of unseen planets and their positions within their... 
waves | hydrodynamics | stars: individual (Elias 2-27, MWC 758) | planet-disk interaction | DENSITY WAVES | ORIGIN | EXCITATION | ASTRONOMY & ASTROPHYSICS | LINDBLAD | CHONDRULES | RESONANCES | Physics - Earth and Planetary Astrophysics
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2017, Volume 850, Issue 2, p. 201
As spiral waves driven by a planet in a gaseous disk steepen into a shock, they deposit angular momentum, opening a gap in the disk. This has been well studied... 
stars: individual (HL Tau, TW Hya, HD 163296) | hydrodynamics | planetdisk interactions | EVOLUTION | IMAGES | ASTRONOMY & ASTROPHYSICS | HL TAU | MASS | ACCRETION | planet-disk interactions | PLANET FORMATION | DISCS | Physics - Earth and Planetary Astrophysics
Journal Article
四川文学, ISSN 1006-8953, 2015, Issue 5, pp. 64 - 65
Journal Article
福建基础教育研究, ISSN 1674-5582, 2015, Issue 11, pp. 110 - 111
地理教学离不开学生对地理事物及现象的感性认识,它是学习地理的一种途径。如何在高中地理教学中增加学生的感性认识呢?在高中地理教学中实施的途径有两条:课堂和课外。 
课堂 | 课外 | 感性认识
Journal Article
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