Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2345..287c&link_type=abstract
In NASA. Goddard Space Flight Center Local Interstellar Medium, No. 81 p 287-296 (SEE N85-15539 06-90)
Astronomy and Astrophysics
Astronomy
2
Electron States, High Temperature Gases, Interstellar Gas, Multiphase Flow, Stellar Spectra, Supernova Remnants, Astronomical Models, Magnetohydrodynamics, Neutron Stars, Stellar Mass Ejection
Scientific paper
The construction of supernova remnant which is consistent with the observations and what it talls about the theory was investigated. It is argued that thermal evaporation and local inhomogeneity are crucial elements which are essential to any satisfactory description. It is concluded that: (1) a multiphase supernova remnant (SNR) seems to provide a plausible description of the local interstellar medium (ISM); (2) the local region could have been deficient in cool gas prior to the supernova both on theoretical and observational grounds; (3) the Sun may lie in a region towards the outside of the supernova remnant which hasn't yet come into pressure equilibrium with the hot gas; and (4) evaporative models give a much more satisfactory description of the O VI observations than Sedov Solutions.
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