SHOCKED INTERSTELLAR GAS IN THE W51 COMPLEX

  • KOO BON-CHUL (Department of Astronomy, Seoul National University)
  • 발행 : 1996.12.01

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.

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