Depletion of elements in shock-driven gas

Details Depletion of elements in shock-driven gas Depletion of elements in shock-driven gas

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.216p..57g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 216, Oct. 1, 1985, p. 57P-63P.

Astronomy and Astrophysics

Astronomy

2

Abundance, Interstellar Gas, Shock Waves, Supernova Remnants, Depletion, Electron Density (Concentration), Gas Density, Silicon, Stellar Mass Ejection

Scientific paper

The depletion of elements in shocked gas in supernova remnants and in interstellar bubbles is examined. It is shown that elements are depleted in varying degrees in gas filaments shocked to velocities up to 200 km s-1 and that large differences in depletions are observed in gas filaments shocked to similar velocities. In the shocked gas the depletion of an element appears to be correlated with the electron density (or the neutral gas density) in the filaments. This correlation, if confirmed, is similar to the correlation between depletion and mean density of gas in the clouds in interstellar space.

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