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Two Remarkably Thin CO Filaments Toward the Supernova Remnant G109.1-1.0
Published online by Cambridge University Press: 12 April 2016
Abstract
We observed the semicircular supernova remnant G109.1-1.0 in the J = 1-0 transition of CO with the Nobeyama 45-m radio telescope. It is found that two remarkably thin molecular filaments delineate the inner boundary of the X-ray jet feature in this remnant. These filaments seem to have experienced evaporation due to the hot gas in the remnant.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 257 - 260
- Copyright
- Copyright © Cambridge University Press 1988