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[KASI Colloquium] October 19 (Wed) 10:30 am - Nguyen Thi Phuong (KASI)
저자 : 한국천문학회 등록일시 : 2022-10-17 12:54:20
첨부파일 :

안녕하십니까.

 

이번주 수요일(10 19) 오전 10:30 아래와 같이 정규 콜로퀴움이 진행될 예정입니다. 많은 참여 부탁드립니다.


발표자 : Nguyen Thi Phuong (KASI Postdoc)

호스트 : 이창원 (전파천문본부)

장소장영실홀 331-2호 및 원격 연결 (대면/비대면 병행)

일시10 19 () 오전 10:30

접속주소https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09

 

제목: Planet formation in a multiple system: gas properties, dynamic and chemical content of GG Tau A

초록

The general picture of planet formation is well agreed: planets are formed within a few million years after the collapse phase in a protoplanetary disk surrounding the protostar. However, the detailed formation conditions and mechanisms are still debated, requiring more sophisticated studies both in theoretical, modeling, and observations. A substantial portion of observed exoplanets is found in binary or higher hierarchical systems. Therefore, studying the physical properties and chemical contents of the protoplanetary disk in binary/multiple systems is essential to understand the formation and variety of planetary systems. I will present a study of GG Tauri A using sub-millimeter observations carried out with ALMA and NOEMA interferometers. GG Tauri A is the prototype of a young triple T Tauri star that is surrounded by a massive and extended Keplerian outer disk. The central cavity is not devoid of gas and dust and at least GG Tauri Aa exhibits its own disk of gas and dust emitting at millimeter wavelengths. Its observed properties make this source an ideal laboratory for investigating planet formation in young multiple solar-type stars. A general picture of gas properties and dynamics from the cavity to outer disk as well as its chemical content and the hint of planet(s) in formation in the circumbinary disk of GG Tau A will be presented.

 

 

진행언어 : 영어

슬라이드언어 : 영어

 

원격 접속 방법 :

A. 웹 브라우저 : Chrome을 추천하며 아래 주소를 실행시 Zoom 구동을 위한 프로그램이 

    설치될 수 있음
B.
접속 주소
https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09
C.
유의사항 : 접속 후 "마이크는 뮤트로 설정" - 기본설정은 뮤트로 되어있음
    >
질의 응답시간에는 마이크를 사용해서 질문 가능함

 

2022년 하반기 KASI 콜로퀴움 일정

https://www.kasi.re.kr/kor/post/eng_colloquium

( 일정은 연사분의 상황에 따라서 변경될 수 있습니다.)

 

천문연 콜로퀴움 위원회 (홍성욱, 최지훈, 오희영드림

 

 

 

Dear all,

 

KASI's regular colloquium is scheduled on this Wednesday, October 19.

 

Speaker : Nguyen Thi Phuong (KASI Postdoc)

Host : Chang-Won Lee

Place : Jang Yeong-sil Hall 331-2 & Online

Time : Oct. 19 (Wed) 10:30 am 

Access: https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09

 

Title: Planet formation in a multiple system: gas properties, dynamic and chemical content of GG Tau A

Abstract: 

The general picture of planet formation is well agreed: planets are formed within a few million years after the collapse phase in a protoplanetary disk surrounding the protostar. However, the detailed formation conditions and mechanisms are still debated, requiring more sophisticated studies both in theoretical, modeling, and observations. A substantial portion of observed exoplanets is found in binary or higher hierarchical systems. Therefore, studying the physical properties and chemical contents of the protoplanetary disk in binary/multiple systems is essential to understand the formation and variety of planetary systems. I will present a study of GG Tauri A using sub-millimeter observations carried out with ALMA and NOEMA interferometers. GG Tauri A is the prototype of a young triple T Tauri star that is surrounded by a massive and extended Keplerian outer disk. The central cavity is not devoid of gas and dust and at least GG Tauri Aa exhibits its own disk of gas and dust emitting at millimeter wavelengths. Its observed properties make this source an ideal laboratory for investigating planet formation in young multiple solar-type stars. A general picture of gas properties and dynamics from the cavity to outer disk as well as its chemical content and the hint of planet(s) in formation in the circumbinary disk of GG Tau A will be presented.

 

Language : English

Slide Language : English

 

Remote access procedure :

 

A. Web browser : Chrome - When executing the address below, a program for additional zoom operation can be installed.

B. Access : Go to  https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09

C. Notice : After join, Please mute your microphone. - The default setting is microphone mute.
     > After the presentation, during the Q&A session, you can use the microphone to ask questions.

 

2022B KASI Colloquium Schedule

https://www.kasi.re.kr/kor/post/eng_colloquium

(This schedule may be changed according to the situation of the speaker.)

 

 

KASI Colloquium committee (Sungwook E. Hong, Jihoon Choi, Heeyoung Oh)

이전글 [KASI Colloquium] September 28 (Wed) 10:30 am - 안성훈 (기초과학연구원) / Tony Ahn (IBS)
다음글 천문학이야기 K-MOOC 강좌
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