The condensation of grains in the ejecta of supernovae

Details The condensation of grains in the ejecta of supernovae The condensation of grains in the ejecta of supernovae

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...157..335p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 157, no. 2, March 1986, p. 335-337.

Astronomy and Astrophysics

Astrophysics

Ejecta, Stellar Envelopes, Stellar Mass Ejection, Supernova Remnants, Astronomical Models, Cosmic Dust, Interstellar Matter, Silicates

Scientific paper

The condensation of grains around supernovae is considered. The
mechanism by which grains could condense from supernovae ejecta to form
a circumstellar dust shell is investigated. It is discovered that the
depletion factor of grain forming material from the surrounding gas is
important.

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