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[KASI Colloquium] May. 7 (Wed.) 4:00 pm - 배영복 박사 (중앙대학교) / Dr. Yeong-Bok Bae (Chung-Ang University)
저자 : 한국천문학회 등록일시 : 2025-05-07 11:04:28
첨부파일 :
 안녕하십니까.

 

오는 수요일(5월 7일) 오후 4:00에 아래와 같이 2025년 상반기 정규 콜로키움이 진행될 예정입니다.

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

 

발표자: 배영복 박사 (중앙대학교)

호스트: 김진호

장소: 장영실홀 331-2 및 원격 연결

일시: 5월 7일 (수) 오후 4:00

접속주소: https://zoom.us/j/96778730290?pwd=guUS8r1bFbggZKMRVcSiTBnIGnZL8p.1

교육학점: 천문연 소속 현장참석자의 경우 필수 0.5 학점 부여

 

제목: Black Hole Binaries as Gravitational-wave sources

초록: 

It has been a decade since the first direct detection of gravitational waves, marking a milestone in astrophysics. Between the first (O1) and third (O3) observing runs, nearly 90 compact binary mergers were identified, with over 90% being binary black hole (BBH) systems. The ongoing fourth observing run (O4), which commenced in May 2023 and is scheduled to conclude in October 2025, continues to expand this catalog.

In this talk, I will provide a broad overview of the formation and evolutionary processes of BBHs through gravitational wave emissions, rather than focusing on a specific detailed topic. Additionally, I will briefly introduce some of my research endeavors related to these phenomena.

 

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://zoom.us/j/96778730290?pwd=guUS8r1bFbggZKMRVcSiTBnIGnZL8p.1

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

 

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

운영위원회 (김진호, 김영민, 이석호, 송영범, 오재석) 

 

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Dear all,

 

The KASI's regular colloquium is scheduled at May. 7, as shown below.

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

 

Speaker: Dr. Yeong-Bok Bae (Chung-Ang University)

Host: Jinho Kim

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

Time: May 7 (Wed) 4:00 pm 

Access: https://zoom.us/j/96778730290?pwd=guUS8r1bFbggZKMRVcSiTBnIGnZL8p.1

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

 

Title: Black Hole Binaries as Gravitational-wave sources

Abstract: 

It has been a decade since the first direct detection of gravitational waves, marking a milestone in astrophysics. Between the first (O1) and third (O3) observing runs, nearly 90 compact binary mergers were identified, with over 90% being binary black hole (BBH) systems. The ongoing fourth observing run (O4), which commenced in May 2023 and is scheduled to conclude in October 2025, continues to expand this catalog.

In this talk, I will provide a broad overview of the formation and evolutionary processes of BBHs through gravitational wave emissions, rather than focusing on a specific detailed topic. Additionally, I will briefly introduce some of my research endeavors related to these phenomena.

 

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://zoom.us/j/96778730290?pwd=guUS8r1bFbggZKMRVcSiTBnIGnZL8p.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, Hyerim Noh, Jeong-Yeol Han)

Working committee (Jinho Kim, Young-Min Kim, Seokho Lee, Youngbum Song, Jae Sok Oh)



이전글 2025 KARI Space Exploration and Science Seminar Series - No.03
다음글 2025 KARI Space Exploration and Science Seminar Series - No.04
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