Fine structure of emission filaments in the Cygnus Loop

Details Fine structure of emission filaments in the Cygnus Loop Fine structure of emission filaments in the Cygnus Loop

Jul 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986afz....25...45k&link_type=abstract

(Astrofizika, vol. 25, July-Aug. 1986, p. 45-55) Astrophysics (ISSN 0571-7132), vol. 25, no. 1, Jan. 1987, p. 381-387. Translati

Astronomy and Astrophysics

Astrophysics

Fine Structure, Interstellar Gas, Interstellar Radiation, Supernova Remnants, Acoustic Propagation, Shock Wave Propagation, Thermal Instability, Wave Equations

Scientific paper

The formation of the fine structure of the emission filaments in the Cygnus Loop by the development of an acoustic mode of thermal instability is considered. Numerical solution of the nonlinear problem has shown that the growth of small adiabatic perturbations can lead to the formation of shock waves if the de-excitation is accompanied by compression of the gas. Such conditions are realized behind the front of a supernova blast wave propagating through inhomogeneous interstellar gas.

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