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Planet のバックアップの現在との差分(No.3)


  • 追加された行はこの色です。
  • 削除された行はこの色です。
#norelated
* 惑星セミナー2016 [#zbb5ecca]
* 惑星セミナー2020 [#zbb5ecca]

惑星セミナーは原則として毎週火曜日の午後14:00から理論部セミナー室で開催しています。~
惑星セミナーは原則として毎週木曜日の14:00から開催しています。(連絡係:星野 遥, 荒川 創太, 古家 健次, 荻原 正博)~
astro-phセミナーは毎週金曜日の12:00から開催しています。(連絡係:Carol Kwok)

// セミナー発表順番
// 脇田->押野->柴田->小久保->荻原->辰馬->瀧->田中
// 

** Schedule & History [#vfafd1d8]

[[2019年度>Planet2019]]
[[2018年度>Planet2018]]
[[2017年度>Planet2017]]
[[2016年度>Planet2016]]
[[2015年度>Planet2015]]
[[2014年度>Planet2014]]

|BGCOLOR(#ccf):|BGCOLOR(#ffc):|BGCOLOR(#cff):|c
|日程|astro-ph|発表|h
|BGCOLOR(#ddf):|BGCOLOR(#ffd):|BGCOLOR(#dff):|c
|[[前期 第1回 4/1>#planet0401]]|||
|[[前期 第2回 4/5>#planet0405]]|押野翔一 (3/14-18)  &br;柴田雄 (3/21-25) &br; 小久保英一郎 (3/28-4/1)||
|[[前期 第3回 4/19>#planet0419]]|脇田茂 (4/4-8)  &br;荻原正博 (4/11-15)||
|[[前期 第4回 4/26>#planet0426]]|瀧哲朗 (4/18-22)|荻原正博&br;「Formation of terrestrial planets in disks evolving via disk winds」|
|[[前期 第5回 5/10>#planet0510]]|田中佑希 (4/25-29)  &br;押野翔一 (5/2-6)||
|[[前期 第6回 5/31>#planet0531]]|小久保英一郎 (5/16-20)  &br;脇田茂 (5/23-27)||
|[[前期 第7回 6/9>#planet0609]]||鈴木建&br;「磁気駆動型円盤風と原始惑星系円盤の進化」|
|[[前期 第8回 6/14>#planet0614]]|柴田雄 (5/9-13)  &br;荻原正博 (5/30-6/3)||
|[[前期 第9回 6/21>#planet0621]]|瀧哲朗 (6/6-10)  &br;田中佑希 (6/13-17) ||
|[[前期 第10回 6/28>#planet0628]]||細野七月&br;「DISPHを用いた、月形成巨大衝突のパラメーターサーベイ」|
|[[前期 第11回 7/5>#planet0705]]|柴田雄 (6/27-7/1) |瀧哲朗&br;「原始惑星系円盤中の圧力バンプにおけるダストの合体成長」|
|[[前期 第12回 7/19>#planet0719]]|押野翔一 (6/20-24)  &br;小久保英一郎 (7/4-8)  &br;脇田茂 (7/11-15)||
|[[前期 第13回 7/26>#planet0726]]|荻原正博 (7/18-22) |田中佑希&br;「ガス惑星大気中における磁気流体波動による惑星風の駆動と加速」|
|[[後期 第1回 10/13>#planet1013]]||Jeroen Bedorf&br;「Using GPU equipped supercomputers for studying the evolution of spiral galaxies」&br;Michiko Fujii&br;「Formation and evolution of spiral arms and bars」|
|[[後期 第2回 10/25>#planet1025]]|瀧哲朗 (9/26-30)  &br;田中佑希 (10/3-7)  &br;押野翔一 (10/10-14) ||
|[[後期 第3回 11/4>#planet1104]]|脇田茂 (10/24-28)||
|[[後期 第4回 11/11>#planet1111]]|小久保英一郎 (10/17-21)  &br;柴田雄 (10/31-11/4)||
|[[後期 第5回 11/24>#planet1124]]|荻原正博 (11/7-11)  &br;辰馬未沙子 (11/14-18)||
|[[後期 第6回 12/6>#planet1206]]|瀧哲朗 (11/21-25)  &br;田中佑希 (11/28-12/2)||
|[[後期 第7回 12/13>#planet1213]]|押野翔一 (12/5-9)|柴田雄&br;「現実的な微惑星集積過程の研究」|
|[[後期 第8回 12/19>#planet1219]]||荒川創太(東工大)&br;「直接合体成長による高空隙率岩石微惑星の形成」|
|[[後期 第9回 12/27>#planet1227]]|小久保英一郎 (12/12-16) &br;脇田茂 (12/19-23) |脇田茂&br;「Numerical studies of planetesimal collisions」|
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|日程|発表|タイトル|Remarks|担当|h
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//|BGCOLOR(#ddf):|BGCOLOR(#ffd):|BGCOLOR(#ffd):|BGCOLOR(#cff):|c
|[[前期 第1回 4/9 15:00->#planet0409]]|All members| Self-introduction |15:00|荻原|
|[[前期 第2回 4/16 14:00->#planet0409]]|Haruka Hoshino, Hirotaka Hohokabe| Small ASJ meeting ||荒川|
|[[前期 第3回 4/23 14:00->#planet0409]]|Yuki Yoshida, Eiichiro Kokubo| Small ASJ meeting ||星野|
|[[前期 第4回 5/14 14:00->#planet0409]]|Sota Arakawa| Thermal history and tidal evolution of trans-Neptunian satellite systems ||古家|
|[[前期 第5回 5/28 14:00->#planet0528]]|Takuya Takarada (ABC)| Radial-velocity search and statistical studies for short-period planets in the Pleiades open cluster ||荒川|
|[[前期 第6回 6/4 16:00->#planet0606]]|Beibei Liu (Lund Univ)| Pebble-driven planet formation around very low-mass stars and brown dwarfs |16:00|荻原|
|[[前期 第7回 7/9 14:00->#planet0606]]|Yuka Fujii|Detecting molecular lines of warm/temperate exoplanets with mid-infrared high-resolution spectroscopy||星野|
|[[前期 第8回 7/21 14:00->#planet0606]]|Masato Ishizuka (U. Tokyo)|Studies of exoplanets with high resolution spectroscopy||古家|

** astro-ph リンク [#gd4ae1b1]

:&aname(planet0405){4/5};|
//今後の候補
//小久保さん:Ishigakiさん(ISAS)
//荻原:駒木さん(東大), Sakurabaさん(東工大), Liu(Lund)
//荒川:本間和明さん(D1)
//古家:野津さん(理研) 
//石澤さん(京大)
//森島さん

押野翔一 (3/14-18)~

- [[Mass constraint for a planet in a protoplanetary disk from the gap width:http://arxiv.org/abs/1603.03853]]

柴田雄 (3/21-25)~
//:&aname(planet1107){5/21}; 名前 タイトル|
//アブスト

- [[Collisionless encounters and the origin of the lunar inclination:http://arxiv.org/abs/1603.06515]]
//:&aname(planet0418){4/18}; Carina Heinreichsberger, Terrestrial or Gaseous? A classification of exoplanets according to density, mass and radius|
//When looking at Exoplanet Archives the class of a planet is not given. Therefore I tried to find an easy and fast way to classify exoplanets using only density, mass and radius. In this talk I will discuss the formation theory of Planets to explain the boundaries between the different classes (gas, terrestrial) and show the results of my empirical study.

小久保英一郎 (3/28-4/1)~
:&aname(planet0604){6/4}; Beibei Liu, Pebble-driven planet formation around very low-mass stars and brown dwarfs|
We conduct a pebble-driven planet population synthesis study to investigate the formation of planets around very low-mass stars and brown dwarfs, in the (sub)stellar mass range between 0.01 M⊙ and 0.1 M⊙. Based on the extrapolation of numerical simulations of planetesimal formation by the streaming instability, we obtain the characteristic mass of the planetesimals and the initial masses of the protoplanets (largest bodies from the planetesimal size distributions), in either the early self-gravitating phase or the later non-self-gravitating phase of the protoplanetary disk evolution. We find that the initial protoplanets form with masses that increase with host mass, orbital distance and decrease with disk age. Around late M-dwarfs of 0.1 M⊙, these protoplanets can grow up to Earth-mass planets by pebble accretion. However, around brown dwarfs of 0.01 M⊙, planets do not grow larger than Mars mass when the initial protoplanets are born early in self-gravitating disks, and their growth stalls at around 0.01 Earth-mass when they are born late in non-self-gravitating disks. Around these low mass stars and brown dwarfs, we find no channel for gas giant planet formation because the solid cores remain too small. When the initial protoplanets form only at the water-ice line, the final planets typically have ≳15% water mass fraction. Alternatively, when the initial protoplanets form log-uniformly distributed over the entire protoplanetary disk, the final planets are either very water-rich (water mass fraction ≳15%) or entirely rocky (water mass fraction ≲5%).

- [[On the Formation of Super-Earths with Implications for the Solar System:http://arxiv.org/abs/1603.08145]]
- [[Ringed Substructure and a Gap at 1 AU in the Nearest Protoplanetary Disk:http://arxiv.org/abs/1603.09352]]
- [[Close-in planets around giant stars. Lack of hot-Jupiters and prevalence of multi-planetary systems:http://arxiv.org/abs/1603.09719]]


:&aname(planet0419){4/19};|

脇田茂 (4/4-8)~

- [[Spontaneous concentrations of solids through two-way drag forces between gas and sedimenting particles:http://arxiv.org/abs/1604.00791]]
- [[The radial dependence of pebble accretion rates: A source of diversity in planetary systems I. Analytical formulation:http://arxiv.org/abs/1604.01291]]

荻原正博 (4/11-15)~

- [[Detection of H2O and evidence for TiO/VO in an ultra hot exoplanet atmosphere:http://arxiv.org/abs/1604.02310]]
- [[A smooth particle hydrodynamics code to model collisions between solid, self-gravitating objects:http://arxiv.org/abs/1604.03290]]
- [[The Impact of Stellar Rotation on the Detectability of Habitable Planets Around M Dwarfs:http://arxiv.org/abs/1604.03135]]
- [[Population synthesis of planet formation using a torque formula with dynamic effects:http://arxiv.org/abs/1604.04116]]
- [[A map of the large day–night temperature gradient of a super-Earth exoplanet:http://www.nature.com/nature/journal/v532/n7598/full/nature17169.html]]


:&aname(planet0426){4/26};|

瀧哲朗 (4/18-22)~

- [[Radiation hydrodynamical models of the inner rim in protoplanetary disks:http://arxiv.org/abs/1604.04601]]
- [[Giant planet formation in radially structured protoplanetary discs:http://arxiv.org/abs/1604.05191]]
- [[ALMA Survey of Lupus Protoplanetary Disks I: Dust and Gas Masses:http://arxiv.org/abs/1604.05719]]
- [[Pebble Accretion and the Diversity of Planetary Systems:Pebble Accretion and the Diversity of Planetary Systems:http://arxiv.org/abs/1604.06362]]


:&aname(planet0510){5/10};|

田中佑希 (4/25-29)~

- [[Photolytic Hazes in the Atmosphere of 51 Eri b:http://arxiv.org/abs/1604.07388]]
- [[Magellan AO System z′, YS, and L′ Observations of the Very Wide 650 AU HD 106906 Planetary System:http://arxiv.org/abs/1604.06847]]
- [[Discovery of a Makemakean Moon:http://arxiv.org/abs/1604.07461]]
- [[The Hunt for Planet Nine: Atmosphere, Spectra, Evolution, and Detectability:http://arxiv.org/abs/1604.07424]]
- [[Lightning as a possible source of the radio emission on HAT-P-11b:http://arxiv.org/abs/1604.07406]]

押野翔一 (5/2-6)~

- [[Secular models and Kozai resonance for planets in coorbital non-coplanar motion:http://arxiv.org/abs/1604.08631]]
- [[Discovery of concentric broken rings at sub-arcsec separations in the HD 141569A gas-rich, debris disk with VLT/SPHERE:http://arxiv.org/abs/1605.00468]]
- [[Survival of habitable planets in unstable planetary systems:http://arxiv.org/abs/1605.01325]]


:&aname(planet0531){5/31};|

小久保英一郎 (5/16-20)~

- [[Dependence of Small Planet Frequency on Stellar Metallicity Hidden by Their Prevalence:http://arxiv.org/abs/1605.04310]]
- [[Habitable Zones of Post-Main Sequence Stars:http://arxiv.org/abs/1605.04924]]
- [[Migration and Growth of Protoplanetary Embryos III: Mass and Metallicity Dependence for FGKM main-sequence stars:http://arxiv.org/abs/1605.05294]]
- [[Red, Rough, Fast, and Perturbed: New Horizons Observations of KBO (15810) 1994 JR1 from the Kuiper Belt:http://arxiv.org/abs/1605.05376]]
- [[Measuring Transit Signal Recovery in the Kepler Pipeline. III. Completeness of the Q1-Q17 DR24 Planet Candidate Catalogue, with Important Caveats for Occurrence Rate Calculations:http://arxiv.org/abs/1605.05729]]

脇田茂 (5/23-27)~

- [[Bayes' theorem and early solar short-lived radionuclides: the case for an unexceptional origin for the solar system:http://arxiv.org/abs/1605.07096]]
- [[Chemical complexity in protoplanetary disks in the era of ALMA and Rosetta:http://arxiv.org/abs/1605.07825]]


:&aname(planet0614){6/14};|

柴田雄 (5/9-13)~

- [[Kepler exoplanets: a new method of population analysis:http://arxiv.org/abs/1605.02255]]
- [[Martian north polar cap summer water cycle:http://arxiv.org/abs/1605.03487]]


荻原正博 (5/30-6/3)~

- [[Free-floating planets from core accretion theory: microlensing predictions:http://arxiv.org/abs/1605.08556]]
- [[No Thermal Inversion and a Solar Water Abundance for the Hot Jupiter HD209458b from HST WFC3 Emission Spectroscopy:http://arxiv.org/abs/1605.08810]]
- [[Examining Tatooine: Atmospheric Models of Neptune-Like Circumbinary Planets:http://arxiv.org/abs/1605.08785]]
- [[HATS-25b through HATS-30b: A Half-dozen New Inflated Transiting Hot Jupiters from the HATSouth Survey:http://arxiv.org/abs/1606.00023]]


:&aname(planet0621){6/21};|

瀧哲朗 (6/6-10)~

- [[A self-consistent model for the evolution of the gas produced in the debris disc of β Pictoris:http://arxiv.org/abs/1606.01247]]
- [[Gap Opening in 3D: Single Planet Gaps:http://arxiv.org/abs/1606.02299]]

田中佑希 (6/13-17)~

- [[EPIC201702477b: A Long Period Transiting Brown Dwarf from K2:http://arxiv.org/abs/1606.04047]]
- [[HAT-P-47b AND HAT-P-48b: Two Low Density Sub-Saturn-Mass Transiting Planets on the Edge of the Period--Mass Desert:http://arxiv.org/abs/1606.04556]]
- [[Search for giant planets in M67 III: excess of hot Jupiters in dense open clusters:http://arxiv.org/abs/1606.05247]]


:&aname(planet0719){7/19};|

押野翔一 (6/20-24)~

- [[A Neptune-sized transiting planet closely orbiting a 5-10-million-year-old star:http://arxiv.org/abs/1606.06729]]
- [[The microlensing rate and distribution of free-floating planets towards the Galactic bulge:http://arxiv.org/abs/1606.06945]]

小久保英一郎 (7/4-8)~

- [[Self-Destructing Spiral Waves: Global Simulations of a Spiral Wave Instability in Accretion Disks:http://arxiv.org/abs/1607.01792]]
- [[Secular resonances with Ceres and Vesta:http://arxiv.org/abs/1607.02035]]
- [[A hot big bang theory: magnetic fields and the early evolution of the protolunar disk:http://arxiv.org/abs/1607.02132]]


脇田茂 (7/11-15)~

- [[Imaging the water-snow line during a protostellar outburst:http://arxiv.org/abs/1607.03757]]


:&aname(planet0726){7/26};|

荻原正博 (7/18-22)~

- [[Constraining the Movement of the Spiral Features and the Locations of Planetary Bodies within the AB Aur System:http://arxiv.org/abs/1607.04280]]
- [[197 Candidates and 104 Validated Planets in K2's First Five Fields:http://arxiv.org/abs/1607.05263]]
 - [[The inclination of the planetary system relative to the solar equator may be explained by the presence of Planet 9:http://arxiv.org/abs/1607.05111]]
- [[Disk Detective: Discovery of New Circumstellar Disk Candidates through Citizen Science:http://arxiv.org/abs/1607.05713]]
- [[Close-in planetesimal formation by pile-up of drifting pebbles:http://arxiv.org/abs/1607.05734]]


:&aname(planet1025){10/25};|

瀧哲朗 (9/26-30)~

- [[Wind-driven Accretion in Transitional Protostellar Disks:https://arxiv.org/abs/1609.07510]]
- [[On dust-gas gravitational instabilities in protoplanetary discs:https://arxiv.org/abs/1609.07930]]
- [[On the origin of horseshoes in transitional discs:https://arxiv.org/abs/1609.08159]]

田中佑希 (10/3-7)~

- [[Possible Internal Structures and Compositions of Proxima Centauri b:https://arxiv.org/abs/1609.09757]]
- [[Rossiter--McLaughlin models and their effect on estimates of stellar rotation, illustrated using six WASP systems:https://arxiv.org/abs/1610.00600]]
- [[VLT FORS2 comparative transmission spectroscopy: Detection of Na in the atmosphere of WASP-39b from the ground:https://arxiv.org/abs/1610.01186]]
- [[Born Dry in the Photo-Evaporation Desert: Kepler's Ultra-Short-Period Planets Formed Water-Poor:https://arxiv.org/abs/1610.01170]]

押野翔一 (10/10-14)~

- [[Are there moonlets near Uranus' alpha and beta rings?:https://arxiv.org/abs/1610.02376]]


:&aname(planet1104){11/4};|

脇田茂 (10/24-28)~

- [[The Spiral Wave Instability Induced by a Giant Planet: I. Particle Stirring in the Inner Regions of Protoplanetary Disks:https://arxiv.org/abs/1610.08502]]


:&aname(planet1111){11/11};|

小久保英一郎 (10/17-21)~

- [[Mass Extinctions and a Dark Disk:https://arxiv.org/abs/1610.04239]]

柴田雄 (10/31-11/4)~

- [[Erosive Hit-and-Run Impact Events: Debris Unbound:https://arxiv.org/abs/1511.04830]]


:&aname(planet1124){11/24};|

荻原正博 (11/7-11)~

- [[Initial mass function of planetesimals formed by the streaming instability:https://arxiv.org/abs/1611.02285]]
- [[Radial Drift of Dust in Protoplanetary Disks: The Evolution of Ice lines and Dead zones:https://arxiv.org/abs/1611.02718]]
- [[Atmospheric Signatures of Giant Exoplanet Formation by Pebble Accretion:https://arxiv.org/abs/1611.03083]]

辰馬未沙子 (11/14-18)~

- [[Rocky Planetesimal Formation via Fluffy Aggregates of Nanograins:https://arxiv.org/abs/1611.03859]]
- [[Photophoretic Levitation and Trapping of Dust in the Inner Regions of Protoplanetary Disks:https://arxiv.org/abs/1611.04610]]
- [[Planetesimal collisions as a chondrule forming event:https://arxiv.org/abs/1611.05511]]


:&aname(planet1206){12/6};|

瀧哲朗 (11/21-25)~

- [[Concentrating small particles in protoplanetary disks through the streaming instability:https://arxiv.org/abs/1611.07014]]

田中佑希 (11/28-12/2)~

- [[Refined architecture of the WASP-8 system: a cautionary tale for traditional Rossiter-McLaughlin analysis:https://arxiv.org/abs/1611.07985]]
- [[An Overabundance of Low-density Neptune-like Planets:https://arxiv.org/abs/1611.09236]]
- [[Hot-Jupiter Core Mass from Roche-lobe Overflow:https://arxiv.org/abs/1611.09373]]
- [[Grand Design Spiral Arms in A Young Forming Circumstellar Disk:https://arxiv.org/abs/1611.09361]]


:&aname(planet1213){12/13};|

押野翔一 (12/5-9)~

- [[Highly inclined and eccentric massive planets. II. Planet-planet interactions during the disc phase:https://arxiv.org/abs/1612.02693]]


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