Far UV nonlinear rise extinction in relation to CH and CH(+) abundances

Details Far UV nonlinear rise extinction in relation to CH and CH(+) abundances Far UV nonlinear rise extinction in relation to CH and CH(+) abundances

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...265l...1j&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 265, no. 1, p. L1-L4.

Astronomy and Astrophysics

Astrophysics

28

Far Infrared Radiation, Hydrocarbons, Interstellar Extinction, Absorption Spectra, Abundance, Cosmic Dust, Interstellar Gas, Interstellar Matter

Scientific paper

The amount of FUV nonlinear rise in the interstellar extinction curve is
found to be proportional to the CH abundance in the line of sight. The
CH(+) abundance shows, if any, a negative trend with the FUV nonlinear
rise. Implications for the carrier of the FUV nonlinear rise are
discussed.

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