Gaseous depletion in the Orion Nebula

Details Gaseous depletion in the Orion Nebula Gaseous depletion in the Orion Nebula

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48..751a&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, Dec. 1977, p. 751-757. In Italian.

Astronomy and Astrophysics

Astronomy

Abundance, Interstellar Gas, Nebulae, Cosmic Dust, Gas-Solid Interfaces, H Ii Regions, Orion Constellation, Oxygen

Scientific paper

The study of gaseous depletion in H II regions is relevant to possible variations of heavy element abundances during the lifetimes of such regions. The present paper develops a theoretical model which attempts to show that there has probably been no significant depletion of oxygen atoms in the Orion nebula by the mechanism of oxygen-atom attachment to dust grains.

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