12月12日（月）13：30～15：00 太陽系小天体セミナー 南棟２階会議室
Dec 12 mon Solar System Minor Body Seminar Conference Room, South Bldg.2F
12月14日（水）10：30～11：30 総研大コロキウム 中央棟（北）1F講義室
Dec 14 wed SOKENDAI Colloquium Lecture room
12月14日（水）13：30～14：30 理論コロキウム コスモス会館会議室
Dec 14 wed DTA colloquium Conference Room, Cosmos Lodge
詳細は以下をご覧下さい。
12月12日（月）
- キャンパス
- 三鷹
- セミナー名
- 太陽系小天体セミナー
- 定例・臨時の別
- 定例
- 日時
- 12月12日（月曜日）13時30分～15時
- 場所
- 南棟２階会議室
- 講演者
- 寺居剛
- 連絡先
- 名前：渡部潤一
- 備考
- テレビ会議またはスカイプによる参加も可
12月14日（水）
- Campus
- Mitaka
- Seminar
- SOKENDAI colloquium
- Regularly Scheduled/Sporadic
- Regularly
- Date and time
- 10:30-11:30, December 14, 2016
- Place
- Lecture Room
- Speaker
- Satoshi Tanioka
- Affiliation
- SOKENDAI M1 (Supervisor; Yoichi Aso)
- Title
- Possible indirect confirmation of the existence of Pop III massive stars by gravitational wave （The review of Kinugawa+14
- Abstract
- (optional)
- Facilitator
- -Name：Kotomi Taniguchi
- Comment
- TV conference system is available connecting from Nobeyama, Hawaii, Mizusawa, and Okayama.
12月14日（水）
- Campus
- Mitaka
- Seminar
- DTA colloquium
- Regularly Scheduled/Sporadic
- Regularly Scheduled Date and time：14 December 2016, 13:30-14:30
- Place
- Conference Room, Cosmos Lodge
- Speaker
- Shunsuke Hozumi
- Affiliation
- Shiga University
- Title
- Intrisic Properties of the Bars Formed by the Bar Instability in Flat Stellar Disks
- Abstract
- Recent observations have revealed that some properties of galactic bars have been uncovered on a statistically meaningful levels of accuracy using a large sample of galaxies. As a result, it has been found that bars in SB0-SBb galaxies are longer than those in SBc to SBd galaxies. Furthermore, also found are such properties that the longer bars have larger amplitudes, and show more elongated shapes. However, these systematic bar properties have never been explained physically. In this talk, I show the properties of the bars formed by the bar instability for flat stellar disk models which are constructed on the basis of exact equilibrium distribution functions. Then, I demonstrate that the properties of the simulated bars are, in large measure, similar to those of the observed bars, and that the amplitude, length, and axis ratio are strongly correlated to an initial typical Toomre’s Q value. Taking into consideration these results, I discuss what the Hubble sequence represents.
- Facilitator
- -Name：Tomoya Takiwaki
- Comment
- in English
以上