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#norelated
* 惑星セミナー2017 [#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。~
// 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]
[[2016年度>Planet2016]]
[[2015年度>Planet2015]]
[[2014年度>Planet2014]]
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|日程|astro-ph|発表|h
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|[[前期 第1回 4/4>#planet0404]]|田中佑希 (3/20-24)|田中佑希 &br;「磁気流体波駆動のガス惑星からの質量放出」|
|[[前期 第2回 4/11>#planet0411]]|押野翔一(3/27-31) &br;柴田雄(4/3-7)|Steven Rieder(AICS, RIKEN)&br;「J1407b: a Super-Saturn or something else?」|
|[[前期 第3回 4/12>#planet0412]]||和田浩二（千葉工大）&br;「ダストアグリゲイトの衝突シミュレーション：成長できるのできないの？」|
|[[前期 第4回 4/25>#planet0425]]|小久保英一郎(4/10-14) &br;脇田茂(4/17-21)|脇田茂&br;「Asteroids and their compositions」|
|[[前期 第5回 5/9>#planet0509]]|荻原正博(4/24-28) &br;辰馬未沙子(5/1-5)||
|[[前期 第6回 5/16>#planet0516]]|瀧哲朗(5/8-12)|押野翔一&br;「High-Resolution N-body Simulations of Planet Formation」|
** astro-ph リンク [#gd4ae1b1]
:&aname(planet0404){4/4};|
田中佑希 (3/20-24)~
- [[Reassessment of the Null Result of the HST Search for Planets in 47 Tucanae:https://arxiv.org/abs/1703.06136]]
- [[Assessing the Habitability of the TRAPPIST-1 System Using a 3D Climate Model:https://arxiv.org/abs/1703.05815]]
- [[The GTC exoplanet transit spectroscopy survey. VII. Detection of sodium in WASP-52b's cloudy atmosphere:https://arxiv.org/abs/1703.06716]]
- [[Formation of TRAPPIST-1 and other compact systems:https://arxiv.org/abs/1703.06924]]
- [[Testing the existence of optical linear polarization in young brown dwarfs:https://arxiv.org/abs/1703.07341]]
- [[The effect of the stellar absorption line centre-to-limb variation on exoplanet transmission spectrum observations:https://arxiv.org/abs/1703.07585]]
- [[Planetesimal formation by the streaming instability in a photoevaporating disk:https://arxiv.org/abs/1703.07895]]
:&aname(planet0411){4/11};|
押野翔一(3/27-31)~
- [[The stability of tightly-packed, evenly-spaced systems of Earth-mass planets orbiting a Sun-like star:https://arxiv.org/abs/1703.08426]]
- [[Water transport to circumprimary habitable zones from icy planetesimal disks in binary star systems:https://arxiv.org/abs/1703.09000]]
- [[Size and density sorting of dust grains in SPH simulations of protoplanetary discs:https://arxiv.org/abs/1703.10385]]
柴田雄(4/3-7)~
- [[The cool and distant formation of Mars:https://arxiv.org/abs/1704.00184]]
:&aname(planet0425){4/25};|
小久保英一郎(4/10-14)~
- [[Plausible Compositions of the Seven TRAPPIST-1 Planets Using Long-term Dynamical Simulations:https://arxiv.org/abs/1704.02261]]
- [[The curiously warped mean plane of the Kuiper belt:https://arxiv.org/abs/1704.02444]]
- [[Limits on the Stability of TRAPPIST-1:https://arxiv.org/abs/1704.02957]]
- [[A Minimum Mass Nebula for M Dwarfs:https://arxiv.org/abs/1704.03265]]
- [[The Destruction of an Oort Cloud in a rich stellar cluster:https://arxiv.org/abs/1704.03341]]
脇田茂(4/17-21)~
- [[Testing the chondrule-rich accretion model for planetary embryos using calcium isotopes:https://arxiv.org/abs/1704.05726]]
:&aname(planet0509){5/9};|
荻原正博(4/24-28)~
- [[Planetary migration and the origin of the 2:1 and 3:2 (near)-resonant population of close-in exoplanets:https://arxiv.org/abs/1704.06459]]
- [[Acceleration of Cooling of Ice Giants by Condensation in Early Atmospheres:https://arxiv.org/abs/1704.07558]]
- [[Titan brighter at twilight than in daylight:https://arxiv.org/abs/1704.07460]]
- [[Avoiding resonance capture in multi-planet extrasolar systems:https://arxiv.org/abs/1704.07836]]
辰馬未沙子(5/1-5)~
- [[3D radiative transfer of intrinsically polarized dust emission based on aligned aspherical grains:https://arxiv.org/abs/1705.01047]]
- [[Survey of cold water lines in protoplanetary disks: indications of systematic volatile depletion:https://arxiv.org/abs/1705.00799]]
- [[A likely detection of a local interplanetary dust cloud passing near the Earth in the AKARI mid-infrared all-sky map:https://arxiv.org/abs/1705.01541]]
:&aname(planet0516){5/16};|
瀧哲朗(5/8-12)~
- [[Composition of Early Planetary Atmospheres II: Coupled Dust and Chemical Evolution in Protoplanetary Disks:https://arxiv.org/abs/1705.02381]]
- [[Chemical enrichment of giant planets and discs due to pebble drift:https://arxiv.org/abs/1705.03305]]
- [[Evidence for universality in the initial planetesimal mass function:https://arxiv.org/abs/1705.03889]]
- [[N-body simulations of planet formation via pebble accretion I: First Results:https://arxiv.org/abs/1705.04264]]
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