오는 수요일(5월 27일) 오후 4:00에 아래와 같이 2026년 상반기 정규 콜로키움이 진행될 예정입니다.

발표 후에는 연사와의 대화시간(5:00-5:40) 및 저녁 식사가 예정되어 있으니 많은 참여 부탁드립니다.

발표자: 권우진 교수 (Seoul National University)

호스트: 이창원

장소: 장영실홀 331-2 및 원격 연결

일시: 5월 27일 (수) 오후 4:00

접속주소: https://us06web.zoom.us/j/84840334355?pwd=3FUkcuaYwNQwscjoUSo3ulk6KPPo6x.1

교육학점: 천문연 소속 현장참석자의 경우 필수 0.5 학점 부여

제목: Structures and Fields in Star Formation

초록: 

Stars form through the gravitational collapse of cold, dense molecular clouds, while planets emerge within the circumstellar disks of protostellar systems. In this talk, I present studies carried out with my students over the past several years to better understand the origins of stars and planets. Using radio observations at (sub)millimeter wavelengths, we investigate both molecular clouds, which define the initial conditions of star formation, and protostellar disks, where planets are born. Particular emphasis will be placed on the role of magnetic fields in molecular clouds as a primary regulator of star formation, as well as on the substructures and grain growth detected in protostellar disks as tracers of early planet formation.

진행언어: 한국어

슬라이드언어: 영어

원격 접속 방법 :

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

B. 접속 주소: https://us06web.zoom.us/j/84840334355?pwd=3FUkcuaYwNQwscjoUSo3ulk6KPPo6x.1

C. 유의사항: 접속 후 "마이크는 뮤트로 설정" - 기본설정은 뮤트로 되어있음 > 질의 응답시간에는 마이크를 사용해서 질문 가능함

천문연 콜로키움 위원회 (김종수, 선광일, 이창원, 문홍규, 한정열, 홍성욱)

운영위원회 (김진호, 홍준석, 석지연, 이재현, 유영삼, 송상헌)

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Dear all,

The KASI's regular colloquium is scheduled at May. 27, as shown below.

A conversation session with speakers and dinner are scheduled after the colloquium.

Speaker: Prof. Woojin Kwon (Seoul National University)

Host: 이창원

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

Time: May 27 (Wed) 4:00 pm 

Access: https://us06web.zoom.us/j/84840334355?pwd=3FUkcuaYwNQwscjoUSo3ulk6KPPo6x.1

KASI Educational credits: 0.5 educational credits are awarded to off-line attendees.

Title: Structures and Fields in Star Formation

Abstract: 

Stars form through the gravitational collapse of cold, dense molecular clouds, while planets emerge within the circumstellar disks of protostellar systems. In this talk, I present studies carried out with my students over the past several years to better understand the origins of stars and planets. Using radio observations at (sub)millimeter wavelengths, we investigate both molecular clouds, which define the initial conditions of star formation, and protostellar disks, where planets are born. Particular emphasis will be placed on the role of magnetic fields in molecular clouds as a primary regulator of star formation, as well as on the substructures and grain growth detected in protostellar disks as tracers of early planet formation.

Language: Korean

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://us06web.zoom.us/j/84840334355?pwd=3FUkcuaYwNQwscjoUSo3ulk6KPPo6x.1

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.

KASI Colloquium committee (Jongsoo Kim, Kwang-Il Seon, Chang Won Lee, Hong-Kyu Moon, Jeong-Yeol Han, Sungwook Hong)

Working committee (Jinho Kim, Junseok Hong,  Ji Yeon Seok, Jaehyun Lee, Young Sam Yu, Sanghun Song)