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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

K. Tatematsu ,
Y. Fukui ,
T. Iwata  and
M. Nakano
K. Tatematsu
Affiliation:
Department of Astrophysics, Faculty of Science, Nagoya University, Chikusa-ku, Nagoya 464, Japan
Y. Fukui
Affiliation:
Department of Astrophysics, Faculty of Science, Nagoya University, Chikusa-ku, Nagoya 464, Japan
T. Iwata
Affiliation:
Department of Astrophysics, Faculty of Science, Nagoya University, Chikusa-ku, Nagoya 464, Japan
M. Nakano
Affiliation:
Department of Earth Science, Faculty of Education, Oita University, Oita 870-11, Japan

Abstract

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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

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