SHOCKED INTERSTELLAR GAS IN THE W51 COMPLEX

BON-CHUL KOO

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SHOCKED INTERSTELLAR GAS IN THE W51 COMPLEX KCI 등재 SCOPUS

BON-CHUL KOO

언어ENG
URLhttps://db.koreascholar.com/Article/Detail/387857

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천문학회지 (Journal of The Korean Astronomical Society)

제29권 제S호 (1996.12)
pp.183-186

한국천문학회 (Korean Astronomical Society)

초록

We report the results of H I 21-cm and molecular line studies of the shocked interstellar gas in the W51 complex. We present convincing evidences suggesting that the shocked gas has been produced by the interaction of the W51C supernova remant (SNR) with a large molecular cloud, Our results show that W51C is the second SNR with direct evidences for the shocked cloud material.

키워드

ISM:individual W51 - ISM:molecules - radio lines - supernova remnants

저자

BON-CHUL KOO(Department of Astronomy, Seoul National University)

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