Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-26T16:19:32.908Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Dickrnan, R.L. 1978, Astrophys. J. Suppl. 37, 407.CrossRefGoogle Scholar
Downes, A. 1983, Monthly Notices Roy. Astron. Soc. 203, 695.CrossRefGoogle Scholar
Fahlman, G.G. and Gregory, P.C. 1981, Nature 293, 202.CrossRefGoogle Scholar
Fahlman, G.G. and Gregory, P.C. 1983, in Supernova Remnants and Their X-Ray Emission, IAU Symp. 101, eds. Danziger, J. and Gorenstein, P. (Reidel, Dordrecht), p. 445.CrossRefGoogle Scholar
Gregory, P.C., Braun, R., Fahlman, G.G., and Gull, S.F. 1983, in Supernova Remnants and Their X-Ray Emission, IAU Symp. 101, eds. Danziger, J. and Gorenstein, P. (Reidel, Dordrecht), p. 437.CrossRefGoogle Scholar
Gregory, P.C. and Fahlman, G.G. 1980, Nature 278, 805 CrossRefGoogle Scholar
Gregory, P.C. and Fahlman, G.G. 1981, Vistas Astron, 54, 229.Google Scholar
Gregory, P.C. and Fahlman, G.G. 1983, in Supernova Remnants and Their X-Ray Emission, IAU Symp. 101, eds. Danziger, J. and Gorenstein, P. (Reidel, Dordrecht), p. 429.CrossRefGoogle Scholar
Heydari-Malayeri, M., Kahane, C., and Lucas, R. 1981, Nature 293, 549.CrossRefGoogle Scholar
Hughes, V.A., Harten, R.H., Costain, C.H., Nelson, L.A., and Viner, M.R. 1984, Astrophys. J. 283, 147 CrossRefGoogle Scholar
Israel, F.P. 1980, Astron. J. 85, 1612.CrossRefGoogle Scholar
Koyama, K., Hoshi, R., and Nagase, F. 1987, submitted to Publ. Astron. Soc. Japan.Google Scholar
Sofue, Y., Takahara, F., and Hirabayashi, H. 1983, Publ. Astron. Soc. Japan 54, 229.Google Scholar
Tatematsu, K., Nakano, M., Yoshida, S., Wiramihardja, S.D., and Kogure, T. 1985, Publ. Astron. Soc. Japan 37, 345.Google Scholar
Tatematsu, K., Fukui, Y., Nakano, M., Kogure, T., Ogavva, H., and Kawabata, K. 1987, Astron. Astrophys. in press.Google Scholar
Tenorio-Tagle, G., Bodenheimer, P., and Yorke, H.W. 1985, Astron. Astrophys. 145, 70 Google Scholar
Weiler, K.W. 1985, in The Crab Nebula and Related Supernova Remnants (eds. Kafatos, M.C. and Henry, R.B.C.) p. 227 (Cambridge University Press, Cambridge).Google Scholar