An interpretation of the semicircular structure of the supernova remnant CTB-109

Details An interpretation of the semicircular structure of the supernova remnant CTB-109 An interpretation of the semicircular structure of the supernova remnant CTB-109

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990acasn..31..121n&link_type=abstract

(Acta Astronomica Sinica, vol. 31, no. 2, 1990, p. 121-127) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 14, Dec. 1

Astronomy and Astrophysics

Astrophysics

2

Molecular Clouds, Stellar Structure, Supernova Remnants, X Ray Sources, Abundance, Diffuse Radiation, Interstellar Gas, Radiation Absorption, Shock Wave Propagation, Thermal Emission

Scientific paper

The supernova explored at the boundary of a dense molecular cloud in a diffuse gas. The eastern half of the shock wave entered the diffuse gas and is now in the stage of adiabatic expansion, forming the observed semicircular remnant; the western half entered the dense cloud, moved at a much slower speed and is now in the pressure-driven snowplow phase, the radiation it emits is in the uv, and is completely absorbed by the interstellar gas along the line of sight.

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