Elemental depletions in single interstellar clouds

Details Elemental depletions in single interstellar clouds Elemental depletions in single interstellar clouds

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...214..304n&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 214, no. 1-2, April 1989, p. 304-306.

Astronomy and Astrophysics

Astrophysics

Abundance, Interstellar Matter, Molecular Clouds, Absorption Spectra, Interstellar Extinction, Spectral Line Width

Scientific paper

The elemental depletion patterns of single interstellar clouds showing different extinction curves and different ratios of diffuse interstellar bands have been studied, based on the intensities of FUV absorption lines of several elements observed with the aid of the Copernicus spectrometer. It is shown that the depletions of certain elements are quite different when observed in clouds, producing different extinction curves and different ratios of the 5780-A and 5797-A diffuse bands. The depletion pattern seems to be very sensitive to the physical parameters of interstellar clouds.

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