The Absorption Feature at 2200 Å in the Interstellar Reddening Curve

Details The Absorption Feature at 2200 Å in the Interstellar Reddening Curve The Absorption Feature at 2200 Å in the Interstellar Reddening Curve

Apr 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..16...75k&link_type=abstract

Astrophysics and Space Science, Volume 16, Issue 1, pp.75-80

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The profile of the absorption feature at 2200 Å has been calculated for model grains of graphite, graphite core-dirty ice mantle and silicate. They are compared with the observed profile obtained by Bless and Savage from a number of early type stars. We have also shown that it is unlikely that the radiation damage of silicates in Interstellar Space can also contribute to the absorption feature at 2200 Å. Lastly, we have discussed briefly how one can meet the objections that have been raised on the silicate model.

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