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* ߥʡ2014 [#rf63bf23]


** Schedule & History [#ac1b69ea]

| 1 4/8|ݱѰϺ (2/24-28)&br;ž (3/17-21)&br;ư (3/24-28)&br; (3/31-4/4)||
| 2 4/15|ͺ (4/7-11)||
|[[ 3 5/13>#planet0513]]|ž (4/14-18)&br;ݱѰϺ (4/21-25)|Ĺëɧ&br;ָϱפˤȤŤshear԰βǽ|
|[[ 4 5/20>#planet0520]]|ư (4/28-5/2)&br; (5/5-9)&br;|߷̲(չ)&br;нˤϵ塢絤ʲ|
|[[ 5 5/30>#planet0530]]|һ (5/12-16)&br;Ĺëɧ (5/19-23)|һ&br;ָξͤȼΥΨοʲˤĤơ|
|[[ 6 6/13>#planet0613]]|ͺ (5/26-30)&br;ž (6/2-6)|ݱѰϺFormation of Close-in Super-Earths by Giant Impacts|
|[[ 7 6/20>#planet0620]]|ݱѰϺ (6/9-13)||
|[[ 8 6/27>#planet0627]]| (6/16-20)|ž&br;֥Ĺˤ Rayleigh-Taylor ԰|
|[[ 9 7/4>#planet0704]]|ư (6/23-27)||
|[[ 10 7/18>#planet0718]]|һ (6/30-7/4)&br;Ĺëɧ (7/7-11)||
|[[ 1 9/5>#planet0905]]|ͺ (7/14-18)&br;ݱѰϺ (7/28-8/1)&br;ư (8/4-8)&br; (8/11-15)&br;һ (8/18-22)&br;Ĺëɧ (8/25-29)||
|[[ 2 9/19>#planet0919]]|ž (7/21-25)&br;ͺ (9/1-5)||
|[[ 3 10/3>#planet1003]]|ž (9/8-12)&br;ݱѰϺ (9/15-19)&br;ư (9/22-26)|&br;Early Solar System Chronology|
|[[ 4 10/10>#planet1010]]| (9/29-10/3)||
|[[ 5 10/17>#planet1017]]|һ (10/6-10)|ư&br;N-body simulation with UPC|
|[[ 6 11/7>#planet1107]]|Ĺëɧ (10/13-17)&br;빾Τ (10/20-24)|ͺ&br;ָμž|
|[[ 7 11/14>#planet1114]]|Ĺë (10/27-31)&br;ž (11/3-7)||
|[[ 8 11/28>#planet1128]]|ͺ (11/10-14)&br;ݱѰϺ (11/17-21)||
|[[ 9 12/5>#planet1205]]|ư (11/24-28)|Ĺëɧ&br;֥Ȥξ˲θפν԰βǽθ˸ơ|
|[[ 10 12/12>#planet1212]]| (12/1-5)||
|[[ 11 12/19>#planet1219]]|һ (12/8-12)||
|[[ 12 1/9>#planet0109]]|Ĺëɧ (12/15-19)&br;  빾 Τ (12/22-26) ||
|[[ 13 1/16>#planet0116]]|Ĺë (12/29-1/2)&br;  ž (1/5-9) ||
|[[ 14 1/23>#planet0123]]|| (NAOJ)&br;ֳֶɥåץ顼ˡˤΥϥӥ֥ϵ巿õ|
|[[ 15 1/30>#planet0130]]|ͺ (1/12-16)|Ĺë&br;Population synthesis calculations: The effect of gas accretion|
|[[ 16 2/6>#planet0206]]|ư (1/26-30)||
|[[ 17 2/13>#planet0213]]|ݱѰϺ (1/19-23)&br;   (2/2-6)|ݱѰϺ&br;Formation of Close-in Super-Earths by Giant Impacts|
|[[ 18 2/20>#planet0220]]|һ (2/9-13)|һ&br;ֽ®٤εʳѤؤαƶ|
|[[ 19 2/27>#planet0227]]||ž&br;֥ؽ԰οͥߥ졼|
|[[ 20 3/6>#planet0306]]|Ĺëɧ (2/16-20)||
|[[ 21 3/13>#planet0313]]&br;(ȹƱ)||ƣǷ(ر)&br;ָϱפξܺٹ¤¿Ĺ¬&br;Man Hoi Lee(The University of Hong Kong)&br;The Puzzle of the Pluto Satellite System|
|[[ 22 3/27>#planet0327]]|빾Τ (2/23-27) &br; Ĺë (3/2-6)&br;  ž (3/9-13)||

** astro-ph  [#i7c44a38]


ž (4/14-18)~
- [[Protoplanetary dust porosity and FU Orionis Outbursts: Solving the mystery of Earth's missing volatiles:http://jp.arxiv.org/abs/1404.3995]]
- [[The ballistic transport instability in Saturn's rings II: nonlinear wave dynamics:http://jp.arxiv.org/abs/1404.4245]]
- [[The ballistic transport instability in Saturn's rings III: numerical simulations:http://jp.arxiv.org/abs/1404.4247]]

ݱѰϺ (4/21-25)~
- [[The Formation of Uranus & Neptune: Challenges and Implications For Intermediate-Mass Exoplanets:http://jp.arxiv.org/abs/1404.5018]]
- [[On the Abundance of Circumbinary Planets:http://jp.arxiv.org/abs/1404.5617]]


ư (4/28-5/2)~
- [[Dancing with the Stars: Formation of the Fomalhaut triple system and its effect on the debris disks:http://jp.arxiv.org/abs/1404.7136]]
- [[On the Spin-axis Dynamics of a Moonless Earth:http://jp.arxiv.org/abs/1404.7505]]

- [[Density, porosity, mineralogy, and internal structure of cosmic dust and alteration of its properties during high velocity atmospheric entry:http://jp.arxiv.org/abs/1405.1596]]
- [[Diversity of planetary systems in low-mass disks: Terrestrial-type planet formation and water delivery:http://jp.arxiv.org/abs/1405.1986]]


һ (5/12-16)~
- [[Secular Effects of Tidal Damping in Compact Planetary Systems:http://jp.arxiv.org/abs/1405.2342]]
- [[Chemistry in an Evolving Protoplanetary Disk: Effects on Terrestrial Planet Composition:http://jp.arxiv.org/abs/1405.3253]]

Ĺëɧ (5/19-23)~
- [[Disc-protoplanet interaction Influence of circumprimary radiative discs on self-gravitating protoplanetary bodies in binary star systems:http://jp.arxiv.org/abs/1405.5056]]


ͺ (5/26-30)~
- [[Impact inducted surface heating by planetesimals on early Mars:http://jp.arxiv.org/abs/1405.5913]]
- [[Planet formation in stellar binaries I: planetesimal dynamics in massive protoplanetary disks:http://jp.arxiv.org/abs/1405.7054]]

ž (6/2-6)~
- [[Modeling dust growth in protoplanetary disks: The breakthrough case:http://jp.arxiv.org/abs/1406.0870]]
- [[Formation of Isothermal Disks around Protoplanets. I. Introductory Three-Dimensional Global Simulations for Sub-Neptune-Mass Protoplanets:http://jp.arxiv.org/abs/1406.0918]]


ݱѰϺ (6/9-13)~
- [[Earthshine on a Young Moon: Explaining the Lunar Farside Highlands:http://jp.arxiv.org/abs/1406.2020]]


- [[Water Ice and Dust in the Innermost Coma of Comet 103P/Hartley 2:http://jp.arxiv.org/abs/1406.3382]]
- [[The Opposition Effect of the Asteroid 4 Vesta:http://jp.arxiv.org/abs/1406.4913]]


ư (6/23-27)~
- [[Global Models of Planet Formation and Evolution:http://jp.arxiv.org/abs/1406.5604]]
- [[A Statistical Reconstruction of the Planet Population Around Kepler Solar-Type Stars:http://jp.arxiv.org/abs/1406.6048]]


һ (6/30-7/4)~
- [[A stellar-mass-dependent drop in planet occurrence rates:http://jp.arxiv.org/abs/1406.7356]]
- [[Explaining Mercury's Density through Magnetic Erosion:http://jp.arxiv.org/abs/1407.0274]]

Ĺëɧ (7/7-11)~
- [[Turbulence-Induced Relative Velocity of Dust Particles III: The Probability Distribution:http://jp.arxiv.org/abs/1407.1101]]


ͺ (7/14-18)~
- [[Water Delivery and Giant Impacts in the 'Grand Tack' Scenario:http://arxiv.org/abs/1407.3290]]
- [[Influence of Stellar Multiplicity On Planet Formation. II. Planets Are Less Common in Multiple-Star Systems with Separations Smaller than 1500 AU:http://arxiv.org/abs/1407.3344]]

ݱѰϺ (7/28-8/1)~
- [[Overcoming the Meter Barrier and The Formation of Systems with Tightly-packed Inner Planets (STIPs):http://arxiv.org/abs/1407.6707]]

ư (8/4-8)~
- [[Dynamical Stability of Terrestrial Planets in the Binary  Centauri System:http://arxiv.org/abs/1408.1053]]
- [[Terrestrial Planet Formation in the Presence of Migrating Super-earths:http://arxiv.org/abs/1408.1215]]

- [[Formation of pebble-pile planetesimals:http://arxiv.org/abs/1408.2535]]
- [[The role of impact and radiogenic heating in the early thermal evolution of Mars:http://arxiv.org/abs/1408.3341]]

һ (8/18-22)~
- [[Towards Chemical Constraints on Hot Jupiter Migration:http://arxiv.org/abs/1408.3668]]
- [[How to reach the orbital configuration of the inner three planets in HD 40307 Planet System ?:http://arxiv.org/abs/1408.4228]]

Ĺëɧ (8/25-29)~
- [[Separating gas-giant and ice-giant planets by halting pebble accretion:http://arxiv.org/abs/1408.6087]]


ž (7/21-25)~
- [[On the Feeding Zone of Planetesimal Formation by the Streaming Instability:http://arxiv.org/abs/1407.5995]]
- [[A six-part collisional model of the main asteroid belt:http://arxiv.org/abs/1407.6143]]

ͺ (9/1-5)~
- [[Stability of the Kepler-11 System and its Origin:http://arxiv.org/abs/1409.0011]]
- [[Understanding the assembly of Kepler's compact planetary systems:http://arxiv.org/abs/1409.0532]]


ž (9/8-12)~
- [[Spherically Symmetric Gravitational Collapse of a Clump of Solids in a Gas:http://arxiv.org/abs/1409.2541]]
- [[How Rocky Are They? The Composition Distribution of Kepler's Sub-Neptune Planet Candidates within 0.15 AU:http://arxiv.org/abs/1409.2982]]

ݱѰϺ (9/15-19)~
- [[Make Super-Earths, Not Jupiters: Accreting Nebular Gas onto Solid Cores at 0.1 AU and Beyond:http://arxiv.org/abs/1409.3578]]
- [[Challenges in Forming the Solar System's Giant Planet Cores via Pebble Accretion:http://arxiv.org/abs/1409.4430]]

ư (9/22-26)~
- [[Terrestrial planet formation in low-mass disks: dependence with initial conditions:http://arxiv.org/abs/1409.7041]]
- [[Planetesimal fragmentation and giant planet formation: the role of planet migration:http://arxiv.org/abs/1409.7102]]


- [[Water Vapour Absorption in the Clear Atmosphere of an exo-Neptune:http://arxiv.org/abs/1409.8349]]
- [[Outward migration of Jupiter and Saturn in 3:2 or 2:1 resonance in radiative disks: implications for the Grand Tack and Nice models:http://arxiv.org/abs/1410.0543]]


һ (10/6-10)~
- [[Formation of close in Super-Earths & Mini-Neptunes: Required Disk Masses & Their Implications:http://arxiv.org/abs/1410.1060]]
- [[Thermal structure of an exoplanet atmosphere from phase-resolved emission spectroscopy:http://arxiv.org/abs/1410.2241]]


Ĺëɧ (10/13-17)~
- [[Can dust coagulation trigger streaming instability?:http://arxiv.org/abs/1410.3832]]
- [[Effects of dust feedback on vortices in protoplanetary disks:http://arxiv.org/abs/1410.4196]]

빾Τ (10/20-24)~
- [[Spin-orbit angle in compact planetary systems perturbed by an inclined companion. Application to the 55 Cancri system:http://arxiv.org/abs/1410.5203]]
- [[Gas and dust structures in protoplanetary disks hosting multiple planets:http://arxiv.org/abs/1410.5963]]


Ĺë (10/27-31)~
- [[Embryo impacts and gas giant mergers II: Diversity of Hot Jupiters' internal structure:http://arxiv.org/abs/1410.6815]]
- [[The stickiness of micrometer-sized water-ice particles:http://arxiv.org/abs/1410.7199]]
- [[Migration and Growth of Protoplanetary Embryos II: Emergence of Proto-Gas-Giants Cores versus Super Earths' Progenitor:http://arxiv.org/abs/1410.7952]]
- [[Radiation-Driven Warping of Circumbinary Disks Around Eccentric Young Star Binaries:http://arxiv.org/abs/1410.8128]]
- [[CO gas inside the protoplanetary disk cavity in HD 142527: disk structure from ALMA:http://arxiv.org/abs/1410.8168]]

ž (11/3-7)~
- [[Collisions of small ice particles under microgravity conditions:http://arxiv.org/abs/1411.0563]]
- [[1D accretion discs around eccentric planets: observable near-infrared variability:http://arxiv.org/abs/1411.1056]]


ͺ (11/10-14)~
- [[Reassessing the formation of the Inner Oort cloud in an embedded star cluster II: Probing the inner edge:http://arxiv.org/abs/1411.1844]]
- [[Migration of massive planets in accreting disks:http://arxiv.org/abs/1411.3190]]

ݱѰϺ (11/17-21)~

- [[Late Accretion and the Late Veneer:http://arxiv.org/abs/1411.4563]]
- [[Chaotic Disintegration of the Inner Solar System:http://arxiv.org/abs/1411.5066]]


ư (11/24-28)~

- [[Detectable close-in planets around white dwarfs through late unpacking:http://arxiv.org/abs/1411.6012]]
- [[Dynamical Interactions Make Hot Jupiters in Open Star Clusters:http://arxiv.org/abs/1411.7061]]



- [[Photophoresis in protoplanetary disks: a numerical approach:http://arxiv.org/abs/1412.1137]]
- [[New insight into the Solar System's transition disk phase provided by the unusual meteorite Isheyevo:http://arxiv.org/abs/1412.1818]]


һ (12/8-12)~

- [[Spiral arms in scattered light images of protoplanetary discs: Are they the signposts of planets?:http://arxiv.org/abs/1412.3412]]
- [[Erosion and the limits to planetesimal growth:http://arxiv.org/abs/1412.3593]]


Ĺëɧ (12/15-19)~

- [[Near-Infrared Image of the Debris Disk around HD 15115:http://arxiv.org/abs/1412.4145]]
- [[Minimum Core Masses for Giant Planet Formation With Realistic Equations of State and Opacities:http://arxiv.org/abs/1412.5185]]

빾 Τ (12/22-26)~

- [[Ammonia, Water Clouds and Methane Abundances of Giant Exoplanets and Opportunities for Super-Earth Exoplanets:http://arxiv.org/abs/1412.7582]]


Ĺë (12/29-1/2)~

- [[Accretion of the Moon from non-canonical disks:http://arxiv.org/abs/1412.8080]]
- [[Halting Migration: Numerical Calculations of Corotation Torques in the Weakly Nonlinear Regime:http://arxiv.org/abs/1412.8092]]

ž (1/5-9)~

- [[Collisions of small ice particles under microgravity conditions (II): Does the chemical composition of the ice change the collisional properties?:http://arxiv.org/abs/1501.00830]]
- [[Sulfurization of Iron in the Dynamic Solar Nebula and Implications for Planetary Compositions:http://arxiv.org/abs/1501.01878]]


ͺ (1/12-16)~

- [[The formation of the solar system:http://arxiv.org/abs/1501.03101]]
- [[Circumbinary planets - why they are so likely to transit:http://arxiv.org/abs/1501.03631]]


ư (1/26-30)~

- [[Gas giant planets as dynamical barriers to inward-migrating super-Earths:http://arxiv.org/abs/1501.06308]]
- [[The Dynamical Evolution of the Asteroid Belt:http://arxiv.org/abs/1501.06204]]


ݱѰϺ (1/19-23)~

- [[The Feeding Zones of Terrestrial Planets and Insights into Moon Formation:http://arxiv.org/abs/1501.03816]]
- [[Giant Planets:http://arxiv.org/abs/1405.3752]]


- [[Compound Chondrules fused Cold:http://arxiv.org/abs/1502.01299]]
- [[Micron-scale D/H heterogeneity in chondrite matrices: a signature of the pristine solar system water?:http://arxiv.org/abs/1502.01067]]


һ (2/9-13)~

- [[Planetary Candidates Observed by Kepler VI: Planet Sample from Q1-Q16 (47 Months):http://arxiv.org/abs/1502.02038]]
- [[Planetary Systems and the Formation of Habitable Planets:http://arxiv.org/abs/1502.02937]]


Ĺëɧ (2/16-20)~

- [[Near-IR imaging of T Cha: evidence for scattered-light disk structures at solar system scales:http://arxiv.org/abs/1502.05084]]


빾Τ (2/23-27)~

- [[The destruction of inner planetary systems during high-eccentricity migration of gas giants:http://arxiv.org/abs/1502.06971]]

Ĺë (3/2-6)~

- [[Combining high-dispersion spectroscopy (HDS) with high contrast imaging (HCI): Probing rocky planets around our nearest neighbors:http://arxiv.org/abs/1503.01136]]
- [[Stellar Multiplicity and Debris Disks: An Unbiased Sample:http://arxiv.org/abs/1503.01320]]

ž (3/9-13)~

- [[Time evolution of snow regions and planet traps in an evolving protoplanetary disk:http://arxiv.org/abs/1503.03352]]

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