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저자 : 한국천문학회 | 등록일시 : 2022-10-17 12:54:20 | |||||||||
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안녕하십니까.
이번주 수요일(10월 19일) 오전 10:30에 아래와
같이 정규 콜로퀴움이 진행될 예정입니다. 많은 참여
부탁드립니다.
호스트 : 이창원 (전파천문본부) 장소 : 장영실홀 331-2호 및 원격 연결 (대면/비대면 병행) 일시 : 10월
19일 (수) 오전 10:30 접속주소 : https://us02web.zoom.us/j/84597516884?pwd=OHVjOEQra1lSZ242K2tOZWY4T2Nzdz09
제목: Planet formation in a multiple system: gas properties,
dynamic and chemical content of GG Tau A 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
2022년 하반기 KASI 콜로퀴움 일정 https://www.kasi.re.kr/kor/post/eng_colloquium (위 일정은
연사분의 상황에 따라서 변경될 수 있습니다.)
천문연 콜로퀴움 위원회 (홍성욱, 최지훈, 오희영) 드림
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.
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) |
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이전글 | [KASI Colloquium] September 28 (Wed) 10:30 am - 안성훈 (기초과학연구원) / Tony Ahn (IBS) |
다음글 | 천문학이야기 K-MOOC 강좌 |